W43A
W43A | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquila |
Right ascension | 18h 47m 40.97s |
Declination | -01° 44′ 55.4″ |
Characteristics | |
Spectral type | OH |
Variable type | Asymptotic giant branch |
Astrometry | |
Radial velocity (Rv) | 13.8 km/s |
Distance | 8500 ly |
Details | |
Other designations | |
Database references | |
SIMBAD | data |
Data sources: | |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
W43A or IRAS 18450-0148 is a late-type star with an envelope of OH/IR type with a magnetically collimated jet (a protoplanetary nebula). The star is in the early stages of becoming a planetary nebula, a process that will take several thousand years.
References
- Vlemmings, Wouter H.T.; Diamond, Philip J.; Imai, Hirosh (2006). "A magnetically collimated jet from an evolved star". Nature. 440 (7080): 58–60. Bibcode:2006Natur.440...58V. doi:10.1038/nature04466. PMID 16511488.
- Imai, Hiroshi; Obara, Kumiko; Diamond, Philip J.; Omodaka, Toshihiro; et al. (2002). "A collimated jet of molecular gas from a star on the asymptotic giant branch". Nature. 417 (6891): 829–831. Bibcode:2002Natur.417..829I. doi:10.1038/nature00788. PMID 12075345.
- Imai, Hiroshi; Nakashima, Jun-ichi; Diamond, Philip J.; Miyazaki, Atsushi; et al. (2005). "A Biconically Expanding Flow in W43A Traced by SiO Maser Emission". The Astrophysical Journal. 622 (2): L125–L128. Bibcode:2005ApJ...622L.125I. doi:10.1086/429820.
- Deacon, R. M.; Chapman, J. M.; Green, A. J.; Sevenster, M. N. (2007). "H2O Maser Observations of Candidate Post-AGB Stars and Discovery of Three High-Velocity Water Sources". The Astrophysical Journal. 658 (2): 1096–1113. arXiv:astro-ph/0702086. Bibcode:2007ApJ...658.1096D. doi:10.1086/511383.
- M. Szymczak & E. Gérard (2004). "Polarimetric observations of OH masers in proto-planetary nebulae". Astronomy & Astrophysics. 423: 209–219. arXiv:astro-ph/0405316. Bibcode:2004A&A...423..209S. doi:10.1051/0004-6361:20040461.
This article is issued from Wikipedia - version of the 10/30/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.