The spectroscopic evolution of the recurrent nova T Pyxidis during its 2011 outburst (Corrigendum). I. The optically thick phase and the origin of moving lines in novae

Details The spectroscopic evolution of the recurrent nova T Pyxidis during its 2011 outburst (Corrigendum). I. The optically thick phase and the origin of moving lines in novae The spectroscopic evolution of the recurrent nova T Pyxidis during its 2011 outburst (Corrigendum). I. The optically thick phase and the origin of moving lines in novae

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012a%26a...537c...2s&link_type=abstract

Astronomy & Astrophysics, Volume 537, id.C2

Astronomy and Astrophysics

Astrophysics

Novae, Cataclysmic Variables, Stars: Individual: T Pyx, Errata, Addenda

Scientific paper

We correct the velocities quoted for interstellar absorption features
from Shore et al. (2011), A&A, 533, L8.

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