X-shooter, NACO, and AMBER observations of the LBV Pistol Star - Archive ouverte HAL
Article Dans Une Revue Bulletin de la Société Royale des Sciences de Liège Année : 2011

X-shooter, NACO, and AMBER observations of the LBV Pistol Star

Résumé

We present multi-instrument and multi-wavelength observations of the famous LBV star Pistol Star. These observations are part of a larger program on early O stars at different metallicities. The Pistol Star has been claimed to be one of the most massive star known, with 250 solar masses. We present preliminary results based on X-shooter spectra, as well as observations performed with the VLTI-AMBER and the VLT-NACO adaptive optics. The X-shooter spectrograph provides simultaneously a spectrum from the UV to the K-band with a resolving power of ˜15000. The preliminary results obtained indicate that Pistol Star has similar properties to eta Car, including shells of matter, but is also a binary.
Fichier non déposé

Dates et versions

hal-03733035 , version 1 (21-07-2022)

Identifiants

Citer

Christophe Martayan, Ronny Blomme, Jean-Baptiste Le Bouquin, Antoine Merand, Guillaume Montagnier, et al.. X-shooter, NACO, and AMBER observations of the LBV Pistol Star. Bulletin de la Société Royale des Sciences de Liège, 2011, 80, pp.400-404. ⟨hal-03733035⟩
27 Consultations
0 Téléchargements

Partager

More