RECENT SCIENTIFIC RESULTS
OBTAINED AT BAO
During the recent years (2000-2008), a number of important results have been
achieved. Altogether, 50 results are
listed, including results in frame of projects that have been started
before and are still active.
1984-2004 Spectroscopic studies of the Second Byurakan Survey galaxies aimed
at study of the sample at B<17; discovery of many new Seyferts, LINERs,
Starbursts, BCDGs, etc. (J.A.
Stepanian, L.K. Erastova, V.H. Chavushian, H.M. Tovmassian, in
collaboration with astronomers from Mexico; S.K.
Balayan, S.A. Hakopian, in collaboration with astronomers from the Special Astrophysical
Observatory, Russia).
J.A. Stepanian, V.H. Chavushyan, L. Carrasco, J.R.
Valdes, R.M. Mujica, H.M. Tovmassian, V.T. Ayvazyan,
Spectral Observations of Faint Markarian Galaxies of the Second Byurakan
Survey. III // Astron. J., Vol. 124, No. 3,
p. 1283-1307, 2002 (and references therein).
S.A. Hakopian, S.K. Balayan, Spectroscopy of Galaxies in Selected Fields of the Second Byurakan
Survey // Astrophysics, Vol. 47, No. 3,
p. 378-388, 2004 (and
references therein).
1984-2002 Study
of the magnetic fields of extragalactic radio sources; correlation between the directions of the magnetic
fields and major axes, mechanism of formation of a dipole magnetic field, etc. (R.R.
Andreasyan, in collaboration with astronomers from France).
R.R.
Andreasyan, S. Appl, H. Sol, Correlation between the
Directions of the Magnetic Fields and Major Axes of Extragalactic Radio Sources
// Astrophysics, Vol. 45, No. 2, p.
198-204, 2002 (and references therein).
1987-2003 The Second part of the FBS, search for blue stellar objects and late-type
stars on the FBS plates. 1103 blue
stellar objects and 1000 late-type stars were revealed, including many new
QSOs, white dwarfs, cataclysmic variables, carbon stars, etc. (H.V. Abrahamian,
A.M. Mickaelian, K.S. Gigoyan, P.K. Sinamyan).
H.V. Abrahamian, A.M. Mickaelian, The
First Byurakan Spectral Sky Survey. Blue Stellar Objects.
XI. Region +80°ЈdЈ+90° // Astrophysics, Vol.
39, No. 4, p. 315-320, 1996 (and references therein).
K.S. Gigoyan, H.V. Abrahamian, et al., First Byurakan
Spectral Sky Survey. Stars of Late-Spectral Types.
XIV. Zone +13°<DEC<+33° // Astrophysics, Vol. 46, No. 4, p. 475-488,
2003 (and references therein). H.V. Abrahamian, 2007, VizieR On-line Data
Catalog: III/246.
1987-2004 Study of Fuors and Subfuors
(Exors); spectral observations of subfuors (E.S.
Parsamian, K.G. Gasparian, in collaboration
with astronomers from Mexico).
E.S.
Parsamian, R. Mujica, L. Corral,
Spectroscopic Observations of Subfuors (Exors). I. V1118 Ori // Astrophyiscs, Vol. 45, No. 4, p. 393-399, 2002.
E.S. Parsamian, R. Mujica,
Spectral Observations of Subfuors (Exors). II. V1143 Ori // Astrophyiscs, Vol. 47, No. 4, p. 433-442, 2004 (and
references therein).
1987-2007 Spectral and photometric study of Shahbazian
compact groups of compact galaxies; it was shown that 7-10% of member
galaxies in Shahbazian compact groups are emission-line galaxies including
classical Sy1-s and narrow-emission-line galaxies (A.S.
Amirkhanian, A.G. Egikian).
A.S.
Amirkhanian, E.Ye. Khachikian, A.G. Eghikian, Spectral and photometric study of compact groups
of compact galaxies // Astrophysics, Vol. 50, No. 3, p. 283-288, 2007 (and
references therein).
1988-2007 Suggestion of new criteria for identification of groups
of galaxies based on the neighbourhood of pairs. Complitaion of a list of galaxy groups. Statistical
investigation of groups (A.P. Mahtessian).
A.P.
Mahtessian, Groups of galaxies. IV. Effect of
observational selection on the relationship between the characteristics and
distance of groups and a comparison with the groups of Geller and Huchra // Astrophysics, Vol. 50, No. 4, p. 440-450,
2007 (and references therein).
1993-2001 Determination of the radio luminosities of pulsars and the distribution
of interstellar electron density based on the pulsars periods and the time
variation of the period. Independent
distances were determined for pulsars and the average electron densities toward
the pulsars were determined from the known dispersion measures. It was shown
that the distribution maximum lies in the vicinity of the Sagittarius spiral
arm (R.R.
Andreasyan, T.G. Arshakian).
R.R.
Andreasyan, T.G. Arshakian, The radio luminosity of pulsars and the
distribution of interstellar electron density // Astrophys. Space Sci., Vol. 278, No. 1/2, p. 175-179, 2001 (and
references therein).
1995-2004 Optical identifications and studies of IRAS
infrared sources. 1577 IRAS point sources were identified
using the FBS spectra and DSS images. Many new IR galaxies (including LIRGs and
ULIRGs, as well as AGNs and interacting/merging pairs and groups) and IR-excess
stars were revealed (A.M. Mickaelian, K.S. Gigoyan, L.A.
Sargsyan).
A.M. Mickaelian, Optical Identifications of the IRAS Point
Sources Based on the First Byurakan Survey // Astrophysics, Vol. 38, No. 4, p. 349-351, 1995.
A.M. Mickaelian, L.A.
Sargsyan, Optical identifications of IRAS Point Sources. Galaxies. X // Astrophysics,
Vol. 47, No. 2, p. 213-228, 2004 (and references therein).
1990s-2001 Studies of the structure of Abell clusters of
galaxies (E.H. Nikogossian).
E.H. Nikogossian, Structure
of the Clusters of Galaxies A 2634, A 1983, and DC 0428-53 // Astrophysics, Vol. 44, No. 3, p. 305-314,
2001 (and references therein).
1990s-2008 Detailed studies of young stellar objects: HH objects, cometary
nebulae, T Tau stars, and associated jets. Studies include imaging, spectroscopic
(including integral field spectroscopy), and near-IR observations (T.Yu. Magakian, T.H. Movsessian, E.H. Nikogossian, E.R. Hovhannessian, in collaboration with astronomers
from Russia, USA, and UK).
T.H. Movsessian, T.Yu.
Magakian, D.M. Sargsyan, E.H. Nikogossian, Integral
spectroscopy of the nebula GM 1-29 and the star PV Cep // Astrophysics, Vol. 51, No. 3, p.
387-393, 2008 (and references therein).
1990s-2007 Multi-wavelength studies of
a new sample of blue compact dwarf
galaxies selected from SBS (A.R.
Petrosian, in collaboration with astronomers from France, Germany, and India).
W.K. Huchtmeier, A.R. Petrosian, Gopal-Krishna, D. Kunth,
HI-observations of blue compact dwarf galaxies.
II // Astron. Astrophys., Vol. 462, No.
3, p. 919-926, 2007 (and references therein).
1990s-2006 Discovery of new dark globules in the star forming regions and
rotation of some of them (A.L.
Gyulbudaghian, in collaboration with astronomers from Spain and Chile).
Carrasco-Gonzalez,
C.; Lopez, R.; A.L. Gyulbudaghian, A.;
Anglada, G.; Lee, C. W., A new radial system of dark
globules in Monoceros // Astron. Astrophys., Vol. 445, No. 3, p. L43-L46, 2006 (and references
therein).
1997-2006 Spectral
investigation of Byurakan-IRAS Galaxies (BIG). (A.M. Mickaelian, S.K. Balayan, S.A.
Hakopian, L.A. Sargsyan, in collaboration with astronomers from France and
Russia).
L.A. Sargsyan, A.M. Mickaelian, Spectral study of BIG objects on the 2.6-m telescope at the Byurakan
Astrophysical Observatory // Astrophysics,
Vol. 49, No. 1, p. 19-35, 2006 (and references therein).
1998-2001 Multiwavelength studies of barred galaxies (A.T.
Kalloghlian, R.A. Kandalyan, V.G. Panajyan, in
collaboration with astronomers from Jordan).
A.T. Kalloghlian, R.A. Kandalyan, H.M.K. Al-Naimiy, A.M. Khassawneh,
Investigation of Barred Galaxies. VII. Comparative Statistics of SB and SA
Galaxies. Near and Mid-IR Regions // Astrophysics,
Vol. 44, No. 3, p. 292-304, 2001 (and references therein).
1999-2001 Discovery of new bright QSOs in the FBS and estimation of their surface
density (0.012 deg-2 for objects with B<16.1). Estimation of the completeness of the Bright Quasar Survey (53%) (A.M.
Mickaelian, in
collaboration with astronomers from France).
A.M. Mickaelian,
A.C. Gonзalves, M.P. Veron-Cetty,
P. Veron, On the nature of the FBS blue stellar
objects and the completeness of the Bright Quasar Survey // Astrophysics,
Vol. 42, No. 1, p. 1-14, 1999.
A.M.
Mickaelian, A.C. Gonзalves, M.P. Veron-Cetty, P. Veron, On the nature of the FBS blue stellar objects and the
completeness of the Bright Quasar Survey. II // Astrophysics, Vol. 44, No. 1, p. 14-22, 2001.
2000 Suggestion of an asymmetric relativistic model for classical
double radio sources based on the statistical analysis of FRII sources from
the 3CRR complete sample (T.G.
Arshakian, in collaboration with M.S. Longair, Cavendish Laboratory, Cambridge
University, UK).
T.G.
Arshakian, M.S. Longair, An asymmetric relativistic model for classical double
radio sources // Mon. Notices Roy.
Astron. Soc., Vol. 311, No. 4, p. 846-860, 2000.
2000-2001 Studies of the relationship between infrared and radio
emission of various types of galaxies, including Seyferts and LINERs (V.H.
Malumian, V.G. Panajyan).
V.H.
Malumian, Relationship Between Infrared and Radio Emission of Spiral Galaxies // Astrophysics, Vol. 43, No. 1, p. 23-31,
2000.
V.H.
Malumian, V.G. Panajyan, Relationship
between Infrared and Radio Emission of Seyfert Galaxies // Astrophysics, Vol. 43, No. 4, p. 403-412, 2000.
V.H.
Malumian, V.G. Panajyan, Relationship
between Infrared and Radio Emission of Galaxies of the LINER Type // Astrophysics, Vol. 44, No. 4, p. 491-497,
2001.
2001 Estimation of the maximum IR luminosity of a single spiral galaxy. It
was shown that all IR sources with luminosities higher than LIR=1012LSun
must be interacting/merging pairs (A.M. Mickaelian, in collaboration with P. Veron and M.P. Veron-Cetty, OHP, France).
A.M. Mickaelian, M.P. Veron-Cetty,
P. Veron, What is the Maximum IR Luminosity of a
Single Spiral Galaxy? // Proc. IAU Symp. 205, ASP, Vol. 205, p. 232-233,
2001.
2001 Discovery of gas-dust shells around 34
early type stars with IR excess based on IRAS observations of O-B-A-F type
stars (R.Kh. Hovhannessian, E.R. Hovhannessian).
R.Kh. Hovhannessian, E.R. Hovhannessian, Gas-Dust Shells around Some Early-Type Stars with an IR Excess (of
Emission) // Astrophysics, Vol. 44, No.
4, p. 454-462, 2001.
2001 Study of the formation of heavy hydrocarbons
in molecular clouds. Laboratory data on the conversion of solid methane
into large hydrocarbons by particle radiation were used to estimate the
fraction of interstellar carbon converted by this process into refractory form (Ar.G. Yeghikian, in collaboration with scientists from University College London, UK).
A.
G. Yeghikyan, S. Viti,
D.A. Williams, The formation of heavy hydrocarbons in molecular clouds // Mon. Notices Roy. Astron. Soc., Vol. 326,
No. 1, p. 313-316, 2001.
2001-2002 Interpretation of the radiation of the coronal supra-thermal streams
by the effect of Compton scattering of the photospheric radiation on fast
electrons of the coronal suprathermal streams (A.G.
Nikoghossian, in collaboration with S. Koutchmy, France).
A.G. Nikoghossian, S. Koutchmy, Interpretation of
the Radiation of Coronal Suprathermal Streams. I // Astrophyiscs, Vol. 44, No. 4, p. 528-535, 2001.
A.G. Nikoghossian, S. Koutchmy,
On Interpretation of the Radiation of Coronal Suprathermal
Streams. II // Astrophyiscs, Vol. 45,
No. 4, p. 489-496, 2002.
2001-2008 Studies of Supernovae in active and
star forming galaxies. Supernovae in isolated galaxies, in pairs and groups
of galaxies. The supernova rate per unit mass. Statistical
investigation of type Ib/c and II supernovae and
their host galaxies. Early-type galaxies with core collapse supernovae (A.R.
Petrosian, et al., in collaboration with astronomers from France,
Italy, and USA).
A.A. Hakobyan, A.R.
Petrosian, B. McLean, D. Kunth,
R.J. Allen, M. Turatto, R. Barbon, Early-type
galaxies with core collapse supernovae // Astronomy
and Astrophysics, Vol. 488, No. 2, p. 523-531, 2008 (and references therein).
2001-2008 Spectral and photometric study of flare stars in Solar neighbourhood and discovery of new flare
stars in Galactic Dark Clouds (N.D.
Melikian, A.A. Karapetian, in collaboration with J.A. Docobo
and V.S. Tamazian, Spain).
N.D. Melikian, V.S. Tamazian,
Spectral and photometric observations of Y Ori // Astrophysics, Vol. 51, No. 4, p. 482-489,
2008 (and references therein).
2001-2008 Study of flare star activity and frequency
distribution of flares. Derivation
of the frequency distribution function of stellar flares and variation in the
flaring activity of flare stars in Pleiades and Orion aggregates (A.A. Akopian).
A. A. Akopian, Long-term
variation in the flaring activity of flare stars // Astrophysics, Vol. 51, No. 1, p. 48-57, 2008 (and references therein).
2002-2003 Extended studies of the Second Byurakan Survey
galaxies (A.R. Petrosian, in collaboration
with Space Telescope Science Institute, USA).
A.R. Petrosian, B. McLean,
R.J. Allen, et al., Studies of the Second Byurakan Survey Galaxies. I. Mergers, Interacting Systems, and Close Pairs // Astron. J., Vol. 123, No. 5, p. 2280-2301,
2002.
A.R. Petrosian, R.J. Allen,
C. Leitherer, et al., Studies of the Second Byurakan Survey Galaxies. II. Comparison of Ultraviolet-excess and Emission-line Techniques // Astron. J., Vol. 125, No. 1, p. 86-97, 2003.
2002-2004 Optical identifications and studies of ROSAT X-ray sources. A large number, 5908 sources from ROSAT-FSC catalogue were identified
using the Hamburg survey spectra and DSS images. The Byurakan/Hamburg/ROSAT Catalogue (BHRC) was
published. 42 new bright AGN were discovered (A.M.
Mickaelian, S.K. Balayan, et al., in collaboration with D. Engels, et
al., Hamburger Sternwarte, Germany).
M.P. Veron-Cetty, S.K. Balayan,
A.M. Mickaelian, et al., Optically
bright AGNs in the ROSAT Faint Source Catalogue // Astron. Astrophys., Vol. 414, p. 487-496, 2004.
A.M. Mickaelian, L.R. Hovhannisyan, D. Engels, H. Hagen, W.
Voges, The Byurakan/Hamburg/ROSAT Catalogue of optical identifications // Astron. Astrophys., Vol. 449, No. 1, p.
425-433, 2006. VizieR On-line Data Catalog:
J/A+A/449/425.
2002-2005 Digitization of the FBS and creation of the largest spectroscopic
database, the Digitized First Byurakan
Survey (DFBS). 20,000,000
low-dispersion spectra (A.M. Mickaelian, L.A. Sargsyan, et
al., in collaboration with
Universita
di Roma “La Sapienza”, Italy and Cornell University,
USA).
A.M. Mickaelian, R. Nesci, C. Rossi, et al., The
Digitized First Byurakan Survey – DFBS // Astron.
Astrophysics, Vol 464, No. 3, p. 1177-1180, 2007.
2002-2008 Many-sided studies of Local Starburst Galaxies. HST/ACS Ly-alpha images of local
starbursts. Extended tidal structure in Ly-alpha-emitting
starbursts. Local Ly-alpha emitters and their
relevance to high-redshift star-forming galaxies. Study
of HII regions in nearby galaxies (A.R. Petrosian, in collaboration
with Space Telescope Science Institute, USA).
J.M.
Mas-Hesse, D. Kunth, H. Atek,
G. Ostlin, C. Leitherer, A.R. Petrosian, D. Schaerer, Local Lyman alpha emitters and their relevance to
high-redshift star-forming galaxies // Astrophys. Space Sci., 2008.
2003 Compilation and
publication of the Merged catalogue of reflection nebulae, the
most complete reference list for these objects (T.Yu. Magakian).
T.Yu. Magakian, Merged catalogue of reflection nebulae // Astron. Astrophys., Vol. 399 No. 1, p.
141-145, 2003. VizieR On-line Data Catalog: J/A+A/399/141.
2003 Obtaining accurate BVIJHK period-luminosity relations
for classical Cepheids in the Galaxy and Magellanic clouds (H.V.
Abrahamian).
H.V.
Abrahamyan, Period-Luminosity Relations for Classical
Cepheids // Astrophysics, Vol. 46, No. 4,
p. 455-464, 2003.
2003 Suggestion of a unified phenomenological model
of light curves of stellar flares to explain a wide variety of flares. An
assumption was made that a flare consists of a fast and relatively strong rise
in brightness followed by a slow and fainter component. The latter is a result
of re-radiation of the part of the energy of the prime flare by the photosphere
of the star (V.P. Zalinian, in collaboration
with astronomers from Mexico).
H.M.
Tovmassian, V.P. Zalinian, N.A. Silant'ev,
O. Cardona, M. Chavez, The unified phenomenological model of light curves of
stellar flares // Astron. Astrophys.,
Vol. 399, No. 2, p. 647-651, 2003.
2003-2007 Detailed study of the T Tau star AA Tau and new T Tau
stars. UBVRI
light curves and magnetospheric accretion-ejection processes in AA Tau (T.Yu. Magakian, et al.,
in collaboration with astronomers from France, Japan, and Kazakhstan).
J.
Bouvier, S.H.P. Alencar, T.
Boutelier, C. Dougados, Z. Balog, K. Grankin, S.T. Hodgkin,
M.A. Ibrahimov, M. Kun, T.Yu.
Magakian, C. Pinte, Magnetospheric accretion-ejection
processes in the classical T Tauri star AA Tauri // Astron. Astrophys., Vol. 463, No. 3, p. 1017-1028, 2007 (and references
therein).
2003-2007 Studies of radio and X-ray
properties of OH megamaser galaxies (R.A. Kandalyan).
R.A. Kandalyan, Some
Features of the X-Ray and Radio Emission from OH Megamaser Galaxies // Astrophysics, Vol. 48, No. 3, p. 355-362,
2005 (and references therein).
2003-2008 Suggestion that cD galaxies are generators of
the clusters in which they occur based on the observed features of cD galaxies and the associated clusters, while all the
galaxies of a given cluster are products of the activity of a central
supergiant galaxy. A physical connection between activity phenomena and cosmic
expansion is sought (H.A. Harutyunian).
H.A.
Harutyunian, Fragmentation of Cosmic Objects in the Course of their Evolution
and the Possible Role of Hubble Expansion in this Process // Astrophysics, Vol. 46, No. 1, p. 81-91,
2003.
H.A.
Harutyunian, On the nature of cD
galaxies // Astrophysics, Vol. 51, No. 2,
p. 141-152, 2008.
2003-2008 Search for Herbig-Haro objects and emission-line stars in star
formation regions. Several dozens of new HH objects and emission stars have
been discovered (T.Yu. Magakian,
T.H. Movsessian, E.H. Nikogossian).
T.H. Movsessian, T.Yu. Magakian, E.H. Nikogossian,
J. Bally, Searches for HH objects and emission stars in star formation
regions. V. Two new cometary nebulae in Perseus // Astrophysics, Vol. 51, No. 2, p. 181-188,
2008 (and references therein).
2003-2008 Detailed investigation of
visual binary stars: orbits, dynamical masses, parallaxes, MK types, etc. (N.D.
Melikian, A.A. Karapetian, in collaboration with
astronomers from Spain and Russia).
J.A.
Docobo, V.S. Tamazian, M. Andrade, N.D. Melikian, A.A. Karapetian, Refining
the Parallax in Visual Double Stars Using Orbital and Spectral Data:
Application to the System of the K0 Giants, A 1808 // Astron. J., Vol. 136, No. 2, p.
890-894, 2008 (and references therein).
2004 The hypothesis of possible anomalous
redshift in spectra of young objects based on counts of faint blue objects,
considered under the assumption that a large fraction of quasars are local objects
ejected from galactic nuclei. This approach was used to examine the problem of
excess of blue galaxies (H.A.
Harutyunian).
H.A.
Harutyunian, Counts of Faint Blue Objects and the Anomalous Red Shift // Astrophysics, Vol. 47, No. 4, p. 538-546,
2004.
2004 A new approach was
proposed for solution of the simplest
one-dimensional problem of diffuse reflection and transmission of radiation in
inhomogeneous atmospheres with finite optical thicknesses, based on
Ambartsumian's method of adding layers. The approach was used to solve the
radiative transfer problem in scattering and absorbing multicomponent
atmospheres (A.G. Nikoghossian).
A.G.
Nikoghossian, Radiative Transfer in Inhomogeneous Atmospheres. I // Astrophysics, Vol. 47, No. 1, p. 104-116,
2004.
A.G.
Nikoghossian, Radiative Transfer in Inhomogeneous Atmospheres. II // Astrophysics, Vol. 47, No. 2, p. 248-259,
2004.
A.G.
Nikoghossian, Radiative Transfer in Inhomogeneous Atmospheres. III // Astrophysics, Vol. 47, No. 3, p. 412-421,
2004.
2004 Statistical studies of properties of SBS galaxies. Diagnostic diagrams and analysis of
activity. Characteristic Features of a separate sample. Distinguishing
active dwarf galaxies (L.K. Erastova).
L.K.
Erastova, Properties of Galaxies in the Second Byurakan Survey. I. Diagnostic
Diagrams // Astrophysics, Vol. 47, No. 1,
p. 79-90, 2004.
L.K.
Erastova, Properties of Galaxies in the Second Byurakan Survey. II.
Characteristic Features of a Separate Sample of Galaxies // Astrophysics, Vol. 47, No. 4, p. 547-554,
2004.
2004 Publication of the Catalog of 216 stars with probable
circular polarization; selection is made from the Catalog of starlight
polarization (7500 stars) (M.H.
Eritsian).
M.A.
Eritsian, Circular Polarization of Starlight // Astrophysics, Vol. 47, No. 3, p. 305-312, 2004. VizieR
On-line Data Catalog: J/other/Ap/47.305.
2004-2006 Statistical studies of pulsars: spatial distribution, age dependence
of several parameters of the radiation, and relation to the supernovae remnants
(V.H.
Malumian, A.N. Harutyunyan).
V.H. Malumian, A.N. Harutyunyan, Spatial Distribution of Pulsars //
Astrophysics, Vol. 47, No. 4, p.
568-572, 2004.
V.H. Malumian, A.N. Harutyunyan, Age Dependence of Several Parameters of the Radiation from Radio Pulsars // Astrophysics,
Vol. 48, No. 2, p. 188-193, 2005.
V.H. Malumian, A.N. Harutyunyan, Relation of pulsars to the remnants of supernova bursts // Astrophysics,
Vol. 49, No. 1, p. 88-95, 2006.
2004-2007 A new survey of cool carbon stars in the halo based on
2MASS. Discovery of very red and distant objects (K.S. Gigoyan, in collaboration
with astronomers from France and UK).
N.
Mauron, M. Azzopardi, K. Gigoyan, T.R. Kendall,
Cool carbon stars in the halo: A new survey based on 2MASS // Astron. Astrophys., Vol. 418, No. 1, p.
77-88, 2004.
N.
Mauron, T.R. Kendall, K. Gigoyan, Cool carbon stars in the
halo. II. A study of 25 new objects // Astron.
Astrophys., Vol. 438, No. 3, p. 867-874, 2005.
N.
Mauron, K. Gigoyan, T.R. Kendall,
Cool carbon stars in the halo: new very red or distant objects // Astron. Astrophys., Vol. 475, No. 3, p.
843-849, 2007.
2004-2008 Studies of the Southern Galactic
molecular clouds and star forming regions. Discovery of new Herbig-Haro objects and outflows (A.L.
Gyulbudaghian, in
collaboration with J. May, et al., Chile).
A.L. Gyulbudaghian, J. May,
Star-forming region BBW 36 in Puppis // Astrophysics, Vol. 51, No. 3, p. 394-402, 2008
(and references therein).
2005 Creation of the Armenian Virtual Observatory (ArVO) and its acceptance in the International Virtual
Observatory Alliance (IVOA) (A.M.
Mickaelian).
A.M. Mickaelian, The
Armenian Virtual Observatory – ArVO // Rom. Astron. J., Vol. 16, p. 23-32, 2006.
2005-2007 Study
of the structure and substructures of
Coma cluster of galaxies. Study of flattening of galaxies
in subclusters of Coma (A.T.
Kalloghlian, in
collaboration with N.G. Kogoshvili
and T.M. Borchkhadze, Georgia).
N.G. Kogoshvili, T.M. Borchkhadze, A.T. Kalloghlian,
Study of the Structure of the Coma Cluster Based on a Hierarchical Force
Clustering Method // Astrophysics, Vol.
48, No. 4, p. 433-444, 2005.
N.G. Kogoshvili, T.M. Borchkhadze, A.T. Kalloghlian,
Flattening of galaxies of different morphological types in subclusters
of Coma // Astrophysics, Vol. 50, No. 3,
p. 289-300, 2007.
2006 Compilation and publication of the Revised and Updated Catalog of the
Byurakan-IRAS Stars (BIS). Multiwavelength data are given for 276 objects (A.M. Mickaelian, K.S. Gigoyan).
A.M. Mickaelian, K.S. Gigoyan, Revised and Updated
Byurakan-IRAS
Star Catalog
// Astron. Astrophysics, Vol.
455, No. 2, p. 765-772, 2006. VizieR On-line
Data Catalog: III/237A.
2006-2008 Spectral investigation of the FBS blue stellar objects; revealing
many new white dwarfs, hot subdwarfs, cataclysmic variables, and a new
planetary nebula. Estimation of the content of the FBS (P.K. Sinamyan,
A.M. Mickaelian).
P.K.
Sinamyan, A.M. Mickaelian, Spectral
observations of blue stellar objects from FBS in the zone d = +43° // Astrophyiscs, Vol. 49, No. 3, p. 333-349, 2006.
P.K.
Sinamyan, A.M. Mickaelian, Spectral
observations of blue stellar objects from FBS in the zone d = +39° // Astrophyiscs, Vol. 51, No. 1, p. 37-47, 2008.
P.K.
Sinamyan, A.M. Mickaelian, Spectral
observations of FBS blue stellar objects in the zone d
= +35° // Astrophyiscs, Vol. 51, No. 2, p. 226-232, 2008.
2007 Compilation and
publication of the Optical Database and
Atlas of Markarian galaxies. Data for 1549 objects are given (A.R.
Petrosian, in collaboration with Space Telescope Science Institute, USA).
A.R. Petrosian,
B. McLean, R.J. Allen, J.W. MacKenty, Markarian
Galaxies. I. The Optical Database and Atlas // Astrophys. J. Suppl., Vol. 170, No. 1, p. 33-70, 2007.
2007 Discovery of 28 highest IR/optical flux
ratio extragalactic objects (having IR/opt up to 1110) by means of
selection of sources from IRAS-FSC and observations with Spitzer Space
Telescope (SST). The sample filled in the gap between the IRAS discovered
ULIRGs and Spitzer discovered 24 mm sources at z~2. The highest luminosity ULIRG was found (1046.6 erg/sec at 5.5 mm) (A.M.
Mickaelian, L.A. Sargsyan, in collaboration with D.W. Weedman and J.R. Houck, Cornell
University, USA).
L.A. Sargsyan, A.M. Mickaelian, D.W. Weedman, J.R.
Houck, Spitzer IRS Spectra of Optically Faint IRAS Sources // Astrophys. J., Vol. 683, No. 1, p. 114-122,
2008.
2008 Compilation and publication of the Revised and Updated Catalog of the FBS blue
stellar objects. Multiwavelength data are given for 1103 objects (A.M. Mickaelian).
A.M. Mickaelian, Revised and Updated Catalogue of the
FBS Blue Stellar Objects // Astron. J.,
Vol. 136, No. 3, p. 946–953, 2008. VizieR On-line Data Catalog: III/258.