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
Scritto
il 10 Gen 2012 alle 01:39
in Pubblicazioni
We correct the velocities quoted for interstellar absorption features
from Shore et al. (2011), A&A, 533, L8.