A SPITZER SEARCH FOR PLANETARY-MASS BROWN DWARFS WITH CIRCUMSTELLAR DISKS: CANDIDATE SELECTION
- 1. Astronomy Department, University of Texas at Austin, 1 University Station C1400, Austin, TX 78712-0259 (United States)
- 2. Department of Physics and Astronomy, Bucknell University, Lewisburg, PA 17837 (United States)
- 3. Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)
Description
We report on initial results from a Spitzer program to search for very low mass brown dwarfs in Ophiuchus. This program is an extension of an earlier study by Allers et al. which had resulted in an extraordinary success rate, 18 confirmed out of 19 candidates. Their program combined near-infrared and Spitzer photometry to identify objects with very cool photospheres together with circumstellar disk emission to indicate youth. Our new program has obtained deep IRAC photometry of a 0.5 deg2 field that was part of the original Allers et al. study. We report 18 new candidates whose luminosities extend down to 10-4 Lsun, which suggests masses down to ∼2 MJ if confirmed. We describe our selection techniques, likely contamination issues, and follow-on photometry and spectroscopy that are in progress.
Availability note (English)
Available from http://dx.doi.org/10.1088/0004-637X/720/2/1374Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 720
- Journal Issue
- 2
- Journal Page Range
- p. 1374-1379
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42055918
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- DWARF STARS; EMISSION; LUMINOSITY; MASS; PHOTOMETRY; PHOTOSPHERE; SPECTROSCOPY; STAR EVOLUTION
- Descriptors DEC
- ATMOSPHERES; EVOLUTION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; SOLAR ATMOSPHERE; STARS; STELLAR ATMOSPHERES