Observations of molecular envelopes of late-type stars: CRL 618, CRL 2688, CRL 3068, and CIT 6

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

27

Carbon Stars, Late Stars, Molecular Gases, Molecular Spectra, Radio Astronomy, Stellar Envelopes, Stellar Evolution, Stellar Spectra, Abundance, Astronomical Spectroscopy, Line Spectra, Planetary Nebulae, Radio Spectra, Radio Telescopes

Scientific paper

The HC3N, HC5N, HC7N, CCH, C4H, SiS, and HNC molecules were observed in the circumstellar envelopes of CRL 618, CRL 2688, CIT 6, and CRL 3068 with the Nobeyama 45 m radio telescope. The observed relative abundances of the cyanopolyynes, CCH, and C4H in these late-type stars are similar to those for IRC +10216. However, it was found that the abundance of HNC increased with the physical evolutionary stage of the stars. In CRL 2688, it is also found that HNC is more concentrated in the inner region than SiS. The production mechanism of HNC is discussed by considering ultraviolet radiation from the central stars. The HC3N J = 4-3 transition was observed to have a P Cygni line profile in CRL 618.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Observations of molecular envelopes of late-type stars: CRL 618, CRL 2688, CRL 3068, and CIT 6 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 Observations of molecular envelopes of late-type stars: CRL 618, CRL 2688, CRL 3068, and CIT 6, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of molecular envelopes of late-type stars: CRL 618, CRL 2688, CRL 3068, and CIT 6 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1326756

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.