STIS spectroscopy of newborn massive stars in SMC N81
arXiv:astro-ph/0110576 · doi:10.1051/0004-6361:20011574
Abstract
Using Hubble Space Telescope observations with STIS, we study the main exciting stars of N81, a high excitation compact Hii region in the Small Magellanic Cloud (SMC). These far UV observations are the first spectroscopic measurements of stars in such a region and reveal features characteristic of an O6-O8 stellar type. The astonishing weakness of their wind profiles and their sub-luminosity (up to ~ 2 mag fainter in Mv than the corresponding dwarfs) make these stars a unique stellar population in the Magellanic Clouds. Our analysis suggests that they are probably in the Hertzsprung-Russell diagram locus of a particularly young class of massive stars, the so-called Vz luminosity class, as they are arriving on the zero age main sequence.
9 pages, 3 figures
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- A Spitzer Space Telescope far-infrared spectral atlas of compact sources in the Magellanic Clouds. I. The Large Magellanic Cloud
- A Spitzer Space Telescope far-infrared spectral atlas of compact sources in the Magellanic Clouds. II. The Small Magellanic Cloud
- The VLT-FLAMES Tarantula Survey. XIII: On the nature of O Vz stars in 30 Doradus
- On the presence and absence of disks around O-type stars
- -band integral field spectroscopy and optical spectroscopy of massive young stellar objects in the Small Magellanic Cloud
- A dearth of young and bright massive stars in the Small Magellanic Cloud
- An interesting candidate for isolated massive star formation in the Small Magellanic Cloud
- A very young component in the pre-eminent starburst region of the Small Magellanic Cloud
- Stellar populations associated with the LMC Papillon Nebula
- The stellar environment of SMC N81
- Low-excitation blobs in the Magellanic Clouds
- The LMC HII region N 214C and its peculiar nebular blob