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

Bibcode
2012A&A...537C...2S
DOI
10.1051/0004-6361/201117721e
Shore, S. N.; Augusteijn, T.; Ederoclite, A.; Uthas, H.
Bibliographical reference

Astronomy and Astrophysics, Volume 537, id.C2

Advertised on:
1
2012
Journal
Astronomy and Astrophysics
Number of authors
4
IAC number of authors
0
Citations
2
Refereed citations
2
Description
We correct the velocities quoted for interstellar absorption features from Shore et al. (2011), A&A, 533, L8.
Type
Erratum
Novae

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