Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-27T00:41:18.387Z Has data issue: false hasContentIssue false
  • English
  • Français

The Blue Stellar Objects of the First Byurakan Survey

Published online by Cambridge University Press:  12 April 2016

A.M. Mickaelian
A.M. Mickaelian*
Affiliation:
Byurakan Astrophysical Observatory (BAO), Byurakan 378433, Armenia. E-mail: [email protected]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Second part of the FBS is devoted to the discovery and study of blue stellar objects. It was carried out in an area of 4009 deg2 and identified 1103 objects: hot subdwarfs and white dwarfs, cataclysmic variables, QSOs and Seyfert galaxies, etc. The discovery of new bright QSOs led to a re-evaluation of their surface density (0.012 deg−2). Several interesting cataclysmic variables have been discovered as well.

Type
Part 1. Optical Surveys for AGN
Information
International Astronomical Union Colloquium , Volume 184: AGN Surveys , 2002 , pp. 101 - 102
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Abrahamian, H.V. et al. 1999, at http://vizier.u-strasbg.fr/ Google Scholar
Mickaelian, A.M. 2000, AATr, 18, 557 Google Scholar
Mickaelian, A.M. et al. 2001a, Ap, 44, 14 Google Scholar
Mickaelian, A.M. et al. 2001b, astro-ph/0108377, A&A (in press)Google Scholar
Schmidt, M., & Green, R.F. 1983, ApJ, 269, 352 Google Scholar
Véron-Cetty, M.-P. & Véron, , 2001, A&A, 374, 92 Google Scholar