A study of RW Ursae Minoris shell

Details A study of RW Ursae Minoris shell A study of RW Ursae Minoris shell

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...364..191e&link_type=abstract

Astronomy and Astrophysics, v.364, p.191-198 (2000)

Astronomy and Astrophysics

Astrophysics

6

Stars: Distances, Stars: Individual: Nova Ursae Minoris 1956, Stars: Individual: Rw Umi, Stars: Novae, Cataclysmic Variables

Scientific paper

We find an expansion parallax for the slow nova RW UMi (Nova Ursae Minoris 1956). A narrow-band Halpha 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 Mv = -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.

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