Context. The Carina Nebula is one of the major massive star-forming regions in the Galaxy.
Its relatively nearby distance (2.35 kpc) makes it an ideal laboratory for the study of massive …

The Carina star-forming region is one of the largest in the Galaxy, and its massive star
population is still being unveiled. The large number of stars combined with high, and highly …

We have obtained multi-epoch observations of 31 O-type stars in the Carina Nebula using
the CHIRON spectrograph on the CTIO/SMARTS 1.5-m telescope. We measure their radial …

We report the discovery of a new O-type double-lined spectroscopic binary with a short
orbital period of 1.4 d. We find the primary component of this binary, FO 15, to have an …

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 …

Aims. We present the first extensive spectroscopic study of the global population in star
clusters Trumpler 16, Trumpler 14, and Collinder 232 in the Carina nebula, using data from …

We present low-resolution optical spectra for 29 X-ray sources identified as either massive
star candidates or low-mass pre-main-sequence (PMS) star candidates in the clusters …

We present the results of a spectroscopic monitoring campaign devoted to three O-type stars
in the Carina nebula. We derive the full SB2 orbital solution of the binary system Tr 16-112 …

We have performed a new abundance analysis of Carina red giant (RG) stars from
spectroscopic data collected with UVES (high spectral resolution) and FLAMES/GIRAFFE …

Context. The Carina Nebula harbors a large population of high-mass stars, including at least
75 O-type and Wolf-Rayet (WR) stars, but the current census is not complete since further …