==========================================================================
J/PASP/117/199 IRTS carbon stars (Le Bertre+, 2005)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
table1.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/PASP/117/199
==========================================================================
drwxr-xr-x 10 cats archive 183 Jan 29 2012 [Up]
drwxr-xr-x 2 cats archive 245 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 472 Dec 19 2022 .message
-r--r--r-- 1 cats archive 5549 Oct 11 2006 ReadMe
-rw-r--r-- 1 cats archive 376 Nov 13 2012 +footg5.gif
-rw-r--r-- 1 cats archive 2999 Nov 13 2012 +footg8.gif
-r--r--r-- 1 cats archive 9080 Mar 6 2006 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/PASP/117/199 IRTS carbon stars (Le Bertre+, 2005)
================================================================================
Carbon stars in the Infrared Telescope in Space Survey.
Le Bertre T., Tanaka M., Yamamura I., Murakami H., MacConnell D.J.
<Publ. Astron. Soc. Pac., 117, 199-206 (2005)>
=2005PASP..117..199L
================================================================================
ADC_Keywords: Stars, carbon ; Photometry, infrared
Abstract:
We have identified 139 cool carbon stars in the near-infrared
spectrophotometric survey of the Infrared Telescope in Space (IRTS)
from the conspicuous presence of molecular absorption bands at 1.8,
3.1, and 3.8mum. Among them, 14 are new bright (K 4.0-7.0) Carbon
stars. We find a trend relating the 3.1mum band strength to the
(K-L') color index, which is known to correlate with mass-loss rate.
This could be an effect of a relation between the depth of the
3.1mum feature and the degree of development of the extended stellar
atmosphere where dust starts to form.