Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.161...99s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 161, no. 1, Nov. 1989, p. 99-109.
Astronomy and Astrophysics
Astrophysics
19
Dark Matter, Spectral Energy Distribution, Star Formation, Cosmic Dust, Interstellar Extinction, Stellar Magnitude, Stellar Spectrophotometry
Scientific paper
The extinction law toward several stars indicating the distance of the Chamaeleon dark cloud was determined. This has also been done for HD 97048 and HD 97300, which turn out to be anomalous with a ratio of total to selective extinction of R about 5.0. In studies involving the distance of the Chamaeleon dark cloud, it is proposed to use 150 + or - 15 pc. The extinction-free spectral energy distribution of HD 97300 does not show the presence of a hot dust shell of 2750 K, which was found by The et al. (1986) in a previous study.
Steenman H.
Thé Pik-Sin
No associations
LandOfFree
Studies of the Chamaeleon star-forming region. III - The distance to the dark cloud and the spectral energy distribution of HD 97048 and HD 97300 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 Studies of the Chamaeleon star-forming region. III - The distance to the dark cloud and the spectral energy distribution of HD 97048 and HD 97300, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Studies of the Chamaeleon star-forming region. III - The distance to the dark cloud and the spectral energy distribution of HD 97048 and HD 97300 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1613000