The nature of V645 Cygni = CRL 2789

Details The nature of V645 Cygni = CRL 2789 The nature of V645 Cygni = CRL 2789

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...215..533c&link_type=abstract

Astrophysical Journal, Part 1, vol. 215, July 15, 1977, p. 533-535, 537-540.

Astronomy and Astrophysics

Astronomy

58

Microwave Spectra, Nebulae, Stellar Evolution, Stellar Spectra, Stellar Winds, Condensation, Cosmic Dust, Millimeter Waves, O Stars, Polarization Characteristics, Radio Sources (Astronomy), Stellar Spectrophotometry

Scientific paper

The rocket-infrared source CRL 2789 coincides with a nebulous object containing a starlike condensation known as V645 Cyg. The nebula shows strong optical polarization. It is interpreted as a bipolar nebula whose central star is invisible directly but whose existence is indicated by scattering from the nebulae. Radio continuum emission is detected at millimeter wavelengths, which is consistent with a free-free spectrum. The system contains an O7 star with a substantial stellar wind, is 6 kpc distant from earth, and consists of a nebulosity with a mean density of 4000 per cu cm containing much denser condensations in which dust grains may be forming. In evolutionary terms, CRL 2789 is a young object.

Affiliated with

Also associated with

No associations

Rating

The nature of V645 Cygni = CRL 2789 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 The nature of V645 Cygni = CRL 2789, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The nature of V645 Cygni = CRL 2789 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1559655