Physics
Scientific paper
May 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33900967b&link_type=abstract
VizieR On-line Data Catalog: J/A+A/390/967. Originally published in: 2002A&A...390..967B
Physics
Stars: Carbon, Stars: Giant, Magnitudes: Absolute, Effective Temperatures
Scientific paper
There are 513 entries corresponding to 513 SEDs of 410 carbon stars and related objects, and 70 Ba II stars. Absolute magnitude bolometric (Col. 7) are given for 348 348 (C & rel.) + 65 (Ba II) entries. Together with the effective temperatures previously obtained (Col. 5), they were used to draw the local HR diagram and the luminosity function for galactic carbon giants and related objects in the Sun vicinity. Also given in column 6, the apparent bolometric magnitudes, and in column 8 as ``remarks'', the variation phase information whenever available, the detection of circumstellar extinction and/or emission, the presence of Tc; the J-type, CH stars, carbon-Cepheids etc., are also shown. Our photometric solutions (photometric type in Col. 3 and interstellar extinction at J in Col. 4: to be multiplied by 1.145 to obtain E(B-V)). (1 data file).
Bergeat J.
Knapik A.
Rutily Bernard
No associations
LandOfFree
Carbon-rich giants in the HR diagram (Bergeat+, 2002) 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 Carbon-rich giants in the HR diagram (Bergeat+, 2002), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Carbon-rich giants in the HR diagram (Bergeat+, 2002) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-834256