Dust and molecules envelope around of RW Cyg

Details Dust and molecules envelope around of RW Cyg Dust and molecules envelope around of RW Cyg

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..366k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 366-367

Computer Science

Scientific paper

IR observations are important for selection dust and molecules in carbon stars. Near IR observations of RW Cyg were obtained by a small IR photometer. Observations were performed at the Peak Terskol Observatory (the Caucasus, H = 3100 m). IR observations confirm the existence of the large dust and molecules envelope with the maximum radiation at 10 micron. Comparison with radio emissions maps and far infrared survey was performed. IR excess may be caused by the C2, CN, HCN molecules and emissions by the CO. Cooperative IR/mm waves observations will be useful for further study of this envelope.

Affiliated with

Also associated with

No associations

Rating

Dust and molecules envelope around of RW Cyg 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 Dust and molecules envelope around of RW Cyg, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dust and molecules envelope around of RW Cyg will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1386861