Spectrum of dust heated by thick accretion disks of pregalactic black holes

Details Spectrum of dust heated by thick accretion disks of pregalactic black holes Spectrum of dust heated by thick accretion disks of pregalactic black holes

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cha%26a..11..234x&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 11, Issue 3, p. 234-236.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We discuss the spectrum of dust heated by accretion disks of SMOs and the effect of the re-radiation on the cosmic muwave background. The main results are: (1) Whether or not there is Lymanalpha cutoff, the dust radiation in the case of SMOs is very strong and will appreciatively distort the muwave background. (2) In spite of (1), the dust radiation spectrum is different when Lyman-α cutoff is present and when it is absent (see Fig.2), and the two cases can be distinguished observationally. An infrared search in the range 200-900 μm would be useful in this connection.

Affiliated with

Also associated with

No associations

Rating

Spectrum of dust heated by thick accretion disks of pregalactic black holes 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 Spectrum of dust heated by thick accretion disks of pregalactic black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrum of dust heated by thick accretion disks of pregalactic black holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1673078