Effective temperatures of carbon-rich stars (Bergeat+, 2001)

Details Effective temperatures of carbon-rich stars (Bergeat+, 2001) Effective temperatures of carbon-rich stars (Bergeat+, 2001)

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ycat..33690178b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/369/178. Originally published in: 2001A&A...369..178B

Physics

Stars: Carbon, Effective Temperatures, Magnitudes

Scientific paper

Table 10 is the full version of Table A1 given in Appendix. There are 441 entries corresponding to 441 spectral energy distributions (SEDs) of 406 carbon stars and related objects studied in Papers I (, II ( and III () (photometric group G in column 3 and extinction A(J) at J-filter in column 4). Two estimates of the effective temperature (Sect. 12) from the SED (calibrated color indices) and bolometric flux (integrated flux: 0.36 to 100μm) are given in columns 5 and 6 respectively, together with the adopted mean value in column 7. Also given in column 8, the apparent bolometric magnitude of the SED/Star, and in column 9 as "remarks", the variation phase information whenever available, the detection of circumstellar extinction and/or emission with associated mbol2 in a few case (see Sect. 13). (2 data files).

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