NGC 330 Be stars and binaries (Martayan+, 2007)

Details NGC 330 Be stars and binaries (Martayan+, 2007) NGC 330 Be stars and binaries (Martayan+, 2007)

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34720577m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/472/577. Originally published in: 2007A&A...472..577M

Physics

Magellanic Clouds, Stars: Be, Stars: Double And Multiple

Scientific paper

Spectra of a significant sample of the B star population in the young cluster SMC NGC 330 and its surrounding field have been obtained with the ESO VLT-FLAMES facilities, as part of the Guaranteed Time Observation programs of the Paris Observatory (P.I.: F. Hammer). The multi-fiber spectrograph VLT-FLAMES has been used in MEDUSA mode (132 fibres) at medium resolution. Observations (ESO runs 72.D-0245A and 72.D-0245C) were carried out on October 21-23, 2003 (blue and red spectra) and on September 9 (blue spectra) and 10, 2004 (red spectra).
(1 data file).

Affiliated with

Also associated with

No associations

Rating

NGC 330 Be stars and binaries (Martayan+, 2007) 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 NGC 330 Be stars and binaries (Martayan+, 2007), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and NGC 330 Be stars and binaries (Martayan+, 2007) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1548850