Open AccessFAUST observations of ultraviolet sources in the directions of NGC 4038–39 and 6752
Author(s) -
Daniels Julian,
Brosch Noah,
Almoznino Elchanan,
Shemmer Ohad,
Bowyer Stuart,
Lampton Michael
Publication year - 2001
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2001.04319.x
Subject(s) - physics , astrophysics , stars , white dwarf , astronomy , spiral galaxy , telescope , globular cluster , halo , galaxy , local group , ultraviolet , galactic halo , dwarf galaxy , quantum mechanics
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.