A study of RW Ursae Minoris shell

ESENOĞLU H. H., SAYGAÇ A. T., Bianchini A., Retter A., ÖZKAN M. T., Altan M.

ASTRONOMY & ASTROPHYSICS, vol.364, no.1, pp.191-198, 2000 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 364 Issue: 1
  • Publication Date: 2000
  • Journal Name: ASTRONOMY & ASTROPHYSICS
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Page Numbers: pp.191-198
  • Keywords: stars : distances, stars : individual : Nova Ursae Minoris 1956, stars : individual : RW UMi, stars : novae, cataclysmic variables, CLASSICAL NOVAE, CATACLYSMIC VARIABLES, EXPANSION PARALLAX, NEBULAR EXPANSION, GALACTIC NOVAE, CATALOG, ATLAS, NOVA-CYGNI-1992, LUMINOSITY, EVOLUTION
  • Anadolu University Affiliated: No

Abstract

We find an expansion parallax for the slow nova RW UMi (Nova Ursae Minoris 1956). A narrow-band H-alpha image shows that the diameter of the nova shell in 1995 was 2.94(+0.37)(-0.49) arcsec. We derive a distance of 5250(+590)(-1050) pc, and an absolute magnitude at maximum of M-v = -7.7(+0.3)(-0.4) which are consistent with previous estimates for the nova. We also revised known relations between various parameters of nova systems.