The discovery of a shell-like event in the O-type star HD 120678

• Published in: Astronomy and astrophysics (Berlin) 2012-10, Vol.546, p.A92
• Main Authors: Gamen, R., Arias, J. I., Barbá, R. H., Morrell, N. I., Walborn, N. R., Sota, A., Maíz Apellániz, J., Alfaro, E. J.
• Format: Article
• Language: English
• Subjects: Astronomy; binaries: spectroscopic; Earth, ocean, space; Exact sciences and technology; stars: early-type; stars: emission-line; stars: individual: HD 120678
• ISSN: 0004-6361; 1432-0746
• DOI: 10.1051/0004-6361/201118725

Aims. We report the detection of a shell-like event in the Oe-type star HD 120678. Methods. HD 120678 has been intensively observed as part of a high-resolution spectroscopic monitoring program of southern Galactic O stars and Wolf-Rayet stars of the nitrogen sequence. Results. An optical spectrogram of HD 120678 obtained in June 2008 shows strong H and He i absorption lines instead of the double-peaked emission profiles observed both previously and subsequently, as well as a variety of previously undetected absorption features, mainly of O ii, Si iii and Fe iii. Photometric data reveal that the development of the absorption spectrum coincided with a remarkable dip in the V-band lightcurve. The “shell phase” of HD 120678 did not persist for very long: the V magnitude recovered its previous average value in fewer than 120 days, whereas H and He emission lines became detectable one year later. Similar spectral variations have been observed in a few Be stars, and they are usually interpreted as changes in the circumstellar disk.