Other
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ycat..73240580d&link_type=abstract
VizieR On-line Data Catalog: J/MNRAS/324/580. Originally published in: 2001MNRAS.324..580D
Other
Photometry: Ultraviolet, Photometry: Ubv
Scientific paper
Analysis of ultraviolet (UV) observations with the FAUST shuttle-borne telescope toward the Antennae and NGC 6752 celestial regions resulted in the detection of 46 and 221 candidate sources respectively, for a signal-to-noise ratio of 8. We discuss the source detection process and the identification of UV sources with optical counterparts. Using correlations with existing catalogues, we present reliable identifications for approximately 60 per cent of the sources. We find that most identified objects are B, A and F stars. The remaining identified objects are galaxies, a white dwarf in a binary system, and two K-type stars. Nearly all of the remaining unidentified objects have assigned optical counterparts but, lacking additional information, we give these only as best estimates. With help from new diagnostic diagrams, we suggest that these unclassified objects are main-sequence (or giant) stars within the local spiral arm or halo; or other hot evolved objects within the local spiral arm. We discuss the nature of the objects found and compare our results with those predicted from spectral and Galactic models. (5 data files).
Almoznino Elchanan
Bowyer Stuart
Brosch Noah
Daniels Jaime
Lampton Michael
No associations
LandOfFree
FAUST sources in NGC 4038-39 and 6752 direction (Daniels+, 2001) 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 FAUST sources in NGC 4038-39 and 6752 direction (Daniels+, 2001), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and FAUST sources in NGC 4038-39 and 6752 direction (Daniels+, 2001) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-820466