Low-mass stars in {sigma} Ori and {lambda} Ori (Sacco+, 2008)

Details Low-mass stars in {sigma} Ori and {lambda} Ori (Sacco+, 2008) Low-mass stars in {sigma} Ori and {lambda} Ori (Sacco+, 2008)

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34880167s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/488/167. Originally published in: 2008A&A...488..167S

Physics

Clusters: Open, Stars: Late-Type, Photometry: Infrared, Spectroscopy

Scientific paper

Observations were carried out using the fiber-fed multi-object spectrograph FLAMES (Fiber Large Array Multi Element Spectrograph), mounted on the UT2 telescope at the VLT and operated in the MEDUSA mode (132 fibers, each with an aperture of 1.2" on the sky).
Observations were performed in service mode and were divided into separate runs of 1h duration each, including instrument overheads. The {sigma} Ori cluster was observed in 6 runs in October and December 2004, while {lambda} Ori was observed in 8 runs in October and November 2005.
(5 data files).

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