Millimetre observations of infrared carbon stars. I. The data

Details Millimetre observations of infrared carbon stars. I. The data Millimetre observations of infrared carbon stars. I. The data

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...390..501g&link_type=abstract

Astronomy and Astrophysics, v.390, p.501-510 (2002)

Astronomy and Astrophysics

Astrophysics

14

Circumstellar Matter, Stars: Mass-Loss, Stars: Agb And Post-Agb

Scientific paper

Millimetre observations of IRAS selected red carbon stars are presented. About 260 stars have been observed with SEST and IRAM in the CO (1-0) and CO (2-1) lines and partially in HCN (1-0) and SiO (3-2). An overall detection rate, in at least one line, of about 80% is achieved. The survey represents the second largest survey for AGB stars, and the largest ever for carbon stars. Two new detections in SiO (3-2) in carbon stars are reported. When available, the SiO/HCN and HCN/CO (1-0) line ratios are consistent with the ratios expected for carbon stars. Based on observations collected at the European Southern Observatory, La Silla, Chile within program ESO 60.E-0103, 62.L-0128, 64.L-0012 and 66.D-0027. Also based on observations with the IRAM telescope, Granada, Spain under programs 98-97, 141-97 and 010-99. The complete Fig. 1 is only available in electronic form at http://www.edpsciences.org. The complete Table 3 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/390/501

Affiliated with

Also associated with

No associations

Rating

Millimetre observations of infrared carbon stars. I. The data 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 Millimetre observations of infrared carbon stars. I. The data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Millimetre observations of infrared carbon stars. I. The data will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1672935