| Issue |
A&A
Volume 537, January 2012
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 1 | |
| Section | Letters | |
| DOI | https://doi.org/10.1051/0004-6361/201117721e | |
| Published online | 09 January 2012 | |
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
1 Dipartimento di Fisica “Enrico Fermi”, Università di Pisa, and INFN- Sezione Pisa, largo B. Pontecorvo 3, 56127 Pisa, Italy
e-mail: shore@df.unipi.it
2 Nordic Optical Telescope, Apartado 474, 38700 Santa Cruz de La Palma, Santa Cruz de Tenerife, Spain
e-mail: tau@not.iac.es
3 Instituto de Astrofísica de Canarias, 38200, La Laguna, Tenerife, Spain
e-mail: ale@iac.es
4 Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
5 Department of Astronomy, Columbia University, 550 W 120th Street, New York, NY 10027, USA
e-mail: helena@astro.columbia.edu
We correct the velocities quoted for interstellar absorption features from Shore et al. (2011), A&A, 533, L8.
Key words: novae, cataclysmic variables / stars: individual: T Pyx / errata, addenda
© ESO, 2012
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