Stellar Parameters and Radial Velocities of Hot Stars in the Carina Nebula
arXiv:1803.05029 · doi:10.3847/1538-3881/aab70d
Abstract
The Carina Nebula is an active star forming region in the southern sky that is of particular interest due to the presence of a large number of massive stars in a wide array of evolutionary stages. Here we present the results of the spectroscopic analysis of 82 B-type stars and 33 O-type stars that were observed in 2013 and 2014. For 82 B-type stars without line blending, we fit model spectra from the Tlusty BSTAR2006 grid to the observed profiles of Hγ and He λλ 4026, 4388, and 4471 to measure the effective temperatures, surface gravities, and projected rotational velocities. We also measure the masses, ages, radii, bolometric luminosities, and distances of these stars. From the radial velocities measured in our sample, we find 31 single lined spectroscopic binary candidates. We find a high dispersion of radial velocities among our sample stars, and we argue that the Carina Nebula stellar population has not yet relaxed and become virialized.
Accepted to AAS Journals (29 pages, 6 figures)
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Cited by in corpus (6)
- A Gaia view of the two OB associations Cygnus OB2 and Carina OB1: The signature of their formation process
- Carina's Pillars of Destruction: the view from ALMA
- Trumpler 16-26: A New Centrifugal Magnetosphere Discovered via SDSS/APOGEE H-band Spectroscopy
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- GG Carinae: orbital parameters and accretion indicators from phase-resolved spectroscopy and photometry
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