21 February 2003 Young Stellar Objects science with interferometry
Author Affiliations +
Abstract
The study of Young Stellar Objects (YSOs) is one of the most exciting topics to be handled by long baseline optical interferometry. The magnitudes of these stars are at the edge of capabilities of current optical interferometers limiting the studies to a few of those but are well within the capability of coming large aperture interferometers like the VLT Interferometer, the Keck Interferometer, the Large Binocular Telescope or 'OHANA. The milli-arcsecond spatial resolution reached by interferometry allows to probe the very close environment of young stars down to a tenth of an astronomical unit. In this paper, I review the different aspects of star formation that can be tackled by interferometry: circumstellar disks, multiplicity, jets, etc. I present recent observations performed with operational infrared interferometers, IOTA, PTI and ISI, and I show why in the next future we will extend these studies with large aperture interferometers.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Fabien Malbet, "Young Stellar Objects science with interferometry", Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); doi: 10.1117/12.458697; https://doi.org/10.1117/12.458697
PROCEEDINGS
13 PAGES


SHARE
RELATED CONTENT

Interferometry on the Large Binocular Telescope
Proceedings of SPIE (October 20 2004)
Keck Interferometer science: present and future
Proceedings of SPIE (October 20 2004)
The Antarctic planet interferometer
Proceedings of SPIE (October 20 2004)
FLUOR fibered beam combiner at the CHARA array
Proceedings of SPIE (February 21 2003)

Back to Top