VizieR Online Data Catalog: BeSOS Be stars stellar parameters (Arcos+, 2018)
Abstract
The observations were carried out using the spectrograph Pontifica Universidad Catolica High Echelle Resolution Optical Spectrograph (PUCHEROS), developed at the Center of Astro-Engineering of Pontifica Universidad Catolica (PUC).
BeSOS observations started in 2012 November. Our programme stars come from a large list of confirmed southern Be stars taken from the Be Star Spectra (BeSS) data base (Neiner et al., 2011AJ....142..149N, http://basebe.obspm.fr) and also a list of B stars showing IR excess taken from the Set of Identifications, Measurements, and Bibliography for Astronomical Data (SIMBAD) data base. (1 data file).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- March 2021
- Bibcode:
- 2021yCat..74745287A
- Keywords:
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- Surveys;
- Stars: Be;
- Effective temperatures;
- Stars: distances;
- Rotational velocities;
- MK spectral classification