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

S. N. Shore¹, T. Augusteijn², A. Ederoclite^3,4 and H. Uthas⁵

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

Abstract

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