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Bright near-infrared sources within 1 deg of the Galactic center. I - Survey and 1-20 micron photometryResults of a near-IR survey of 0.55 sq deg toward the Galactic center are reported. Additional IR photometry of 50 objects found in this survey was made in order to investigate the nature of luminous stars in the central region of the Milky Way including all sources with K less than 7.6 and H-K not less than 1.4. In addition to candidates for normal M-type stars and long-period variables, four objects whose energy spectra peak at about 5 microns have been detected in a small region around (l, b) = (0.15, 0.0 deg), near the crossing of the 6-cm radio arc with the Galactic plane. These four might be young stellar objects near the Galactic center. It is suggested that the relative depth change in the silicate absorption is localized to a fairly small region around the Galactic center.
Document ID
19930049509
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Nagata, Tetsuya
(Kyoto Univ. Japan; Mount Stromlo and Siding Spring Observatories, Canberra, Australia; NASA, Infrared Telescope , United States)
Hyland, A. R.
(NASA Headquarters Washington, DC United States)
Straw, S. M.
(Mount Stromlo and Siding Spring Observatories Canberra, Australia)
Sato, Shuji
(National Astronomical Observatory, Mitaka; Kyoto Univ. Japan)
Kawara, Kimiaki
(National Astronomical Observatory, Mitaka, Japan; Mount Stromlo and Siding Spring Observatories Canberra, Australia)
Date Acquired
August 16, 2013
Publication Date
April 1, 1993
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 406
Issue: 2
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
93A33506
Funding Number(s)
CONTRACT_GRANT: NSF AST-84-20775
Distribution Limits
Public
Copyright
Other

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