Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acaps...4...89t&link_type=abstract
(Acta Astrophysica Sinica, vol. 4, 1984, p. 89-96) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 8, Dec. 1984, p. 34
Astronomy and Astrophysics
Astrophysics
Hydroxyl Emission, Infrared Radiation, Interstellar Masers, Variable Stars, Density Distribution, Luminosity, Mira Variables, Radiant Flux Density, Spatial Distribution
Scientific paper
Published observational data on 127 OH-maser sources for which visible or IR identifications and distance estimates are available (mainly from the list of Engels, 1979) are analyzed statistically to determine their Galactic distribution and luminosity function. The results are presented graphically and discussed. A density distribution with a steep peak at about 7.5 kpc from the Galactic center and FWHM 2.1 kpc, similar to that found for Mira variables by Glass et al. (1982) and markedly different from that of Baud et al. (1979 and 1981) for unidentified objects, is observed. The luminosity function rho(L) is found to be equal to 189.67 L exp -1.79, like that for unidentified objects, despite the fact that the observed luminosity range (0.16-1000 Jy kpc sq) of the identified sources is wider than that determined by Bowers (1978) for unidentified sources.
Sun Juanjuan
Tong Yu
Xie Shu-Ding
Yang Xiaoping
No associations
LandOfFree
Spatial distribution and luminosity function of OH/IR maser sources does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Spatial distribution and luminosity function of OH/IR maser sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spatial distribution and luminosity function of OH/IR maser sources will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-733216