The spectroscopic evolution of V5584 Sgr (Nova Sgr 2009 No. 4)

Details The spectroscopic evolution of V5584 Sgr (Nova Sgr 2009 No. 4) The spectroscopic evolution of V5584 Sgr (Nova Sgr 2009 No. 4)

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.333..115p&link_type=abstract

Astrophysics and Space Science, Volume 333, Issue 1, pp.115-118

Astronomy and Astrophysics

Astrophysics

Stars: Novae, Cataclysmic Variables

Scientific paper

We have secured optical spectroscopy of the nova V5584 Sgr at the Loiano Observatory, Italy, during the post outburst decline. V5584 Sgr showed the presence of nebular lines. We have estimated the decline time by two magnitudes, 27 days, the absolute magnitude at maximum, -7.2 to -7.7, the white dwarf mass, 0.8 to 0.9 M &sun;, the distance, 5.8 to 7.1 kpc.

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