Intrinsically polarized stars and implication for star formation in the central parsec of our galaxy
- 1. Department of Astronomy, Graduate School of Science, Kyoto University, Kyoto 606-8502 (Japan)
- 2. National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan)
- 3. Subaru Telescope, National Astronomical Observatory of Japan, 650 North A'ohoku Place, Hilo, HI 96720 (United States)
Description
We have carried out adaptive-optics assisted observations at the Subaru Telescope and have found 11 intrinsically polarized sources in the central parsec of our Galaxy. They are selected from 318 point sources with KS < 15.5, and their interstellar polarizations are corrected using a Stokes Q/I-U/I diagram. Considering brightness, near-infrared color excess, and the amount of intrinsic polarization, two of them are good young stellar object (YSO) candidates with an age of ∼105 yr. If they are genuine YSOs, their existence provides strong constraints on star formation mechanisms in this region. In the remaining sources, two are known as bow-shock sources in the Northern Arm. One other is also located in the Northern Arm and shows very similar properties, and thus it is likely to be a so far unknown bow-shock source. The origin of the intrinsic polarization of the other sources is as yet uncertain.
Availability note (English)
Available from http://dx.doi.org/10.1088/0004-637X/778/2/92Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 778
- Journal Issue
- 2
- Journal Page Range
- [10 p.]
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 46048299
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BRIGHTNESS; COLOR; GALAXIES; LIMITING VALUES; POINT SOURCES; POLARIZATION; SHOCK WAVES; STARS; TELESCOPES
- Descriptors DEC
- OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; RADIATION SOURCES