Optical Identification of IRAS Point Sources. Galaxies. X

Springer Science and Business Media LLC - Tập 47 - Trang 213-228 - 2004
A. M. Mickaelian1, L. A. Sargsyan1
1V. A. Ambartsumyan Byurakan Astrophysical Observatory, Armenia

Tóm tắt

The tenth list of objects from the BIG (Byurakan-IRAS Galaxies) sample, containing 104 galaxies identified with 60 point sources from the IRAS PSC catalog, is introduced. The identifications have been made in the region +69°≤δ≤+73° and 09h50m≤α≤15h20m with an area of 107 sq.deg. The identified objects include 13 Sy candidates, 5 compact star-formation galaxies, 11 interacting pairs (including 5 “merger” candidates) and 1 interacting triple system, 5 LSB galaxies, and 5 groups. 21 objects are also identified with radio sources. The optical coordinates, their deviations from the IR coordinates, V stellar magnitudes, morphological types, angular sizes of the central regions, and position angles have been determined. The identified galaxies are of Sa-Sc, SB, and Irr morphological types, the optical stellar magnitudes lie in the range 15m.0-21m.5, and the angular sizes of the central regions lie in the range 3″-32″. Finding charts from the DSS2 are included for these objects.

Tài liệu tham khảo

B. E. Markarian, V. A. Lipovetski, J. A. Stepanian, et al., Commun. Special Astrophys. Observ. 62, 5 (1989). A. M. Mickaelian, Astrofizika 38, 625 (1995). Joint IRAS Science Working Group. Infrared Astronomical Satellite Catalogs, The Point Source Catalog Version 2. 0, NASA RP-1190 (1988). M. Moshir, G. Kopan, T. Conrow, et al., Infrared Astronomical Satellite Catalogs, The Faint Source Catalog, Version 2. 0 (1990). T. McGlynn, N. E. White, and K. Scollick, ASP Conf. Ser. 61, 34 (1994). DSS2, The Second Generation Digitized Sky Survey, STScI, at http://stdatu.stsci.edu/cgi-bin/dss_form. A. M. Mickaelian and L. A. Sargsyan, Astrofizika 47, 109 (2004). A. M. Mickaelian and K. S. Gigoyan, Astrofizika 44, 222 (2001). J. J. Condon, W. D. Cotton, E. W. Greisen, et al., Astron. J. 115, 1693 (1998). M. P. Veron-Setti and F. Veron, personal communication (1999). I. R. King and M. J. Raff, Publ. Astron. Soc. Pacif. 89, 120 (1977). R. L. Pennington, R. M. Humphreys, S. C. Odewahn, et. al., Publ. Astron. Soc. Pacif. 105, 521 (1993); http:// aps.umn.edu/. D. Monet, A. Bird, B. Canzian, et al., USNO-SA2. 0 (U. S. Naval Observ., Washington DC) (1996). D. B. Sanders and I. F. Mirabel, Luminous Infrared Galaxies, Ann. Rev. Astron. Astrophys. 34, 749 (1996). A. R. Klemola, B. F. Jones, and R. B. Hanson, Astron. J. 94, 501 (1987). W. Voges, W. Aschenbach, T. Boller, et al., Astron. Astrophys. 349, 389 (1999). P. C. Gregory, W. K. Scott, K. Douglas, and J. J. Condon, Astrophys. J. Suppl. Ser. 103, 427 (1996). J. N. Douglas, F. N. Bash, F. A. Bozyan, et al., Astron. J. 111, 1945 (1996). R. B. Rengelink, Y. Tang, A. G. De Bruyn, et al., Astron. Astrophys. Suppl. Ser. 124, 259 (1997).