lam Ori and sig Ori low-mass stars spectroscopy (Maxted+, 2008)

Details lam Ori and sig Ori low-mass stars spectroscopy (Maxted+, 2008) lam Ori and sig Ori low-mass stars spectroscopy (Maxted+, 2008)

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..83852210m&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/385/2210. Originally published in: 2008MNRAS.385.2210M

Physics

Binaries: Spectroscopic, Radial Velocities, Spectroscopy

Scientific paper

Radial velocities and spectral indices for 218 stars and brown dwarfs around {sigma} and {lambda} Orionis. Observations were obtained with the FLAMES/GIRAFFE multi-object spectrograph on ESO's VLT UT2 (Kueyen) telescope (programme ID 076.C_145). The equivalent width of the NaI 8200{AA} and the strength of the TiO 8442{AA} spectral features were measured from the median average spectrum. Radial velocities were measured by cross-correlation against a template spectrum of the brown dwarf star USco CTIO 055 at multiple epochs.
(3 data files).

Affiliated with

Also associated with

No associations

Rating

lam Ori and sig Ori low-mass stars spectroscopy (Maxted+, 2008) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with lam Ori and sig Ori low-mass stars spectroscopy (Maxted+, 2008), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and lam Ori and sig Ori low-mass stars spectroscopy (Maxted+, 2008) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1077976