==========================================================================
J/MNRAS/394/795 AGN in Fornax dwarf spheroidal galaxy (Whitelock+, 2009)
The following files can be converted to FITS (extension .fit or fit.gz)
table1.dat table[23].dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/394/795
==========================================================================
drwxr-xr-x 16 cats archive 282 Jul 9 2015 [Up]
drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 483 Dec 19 2022 .message
-r--r--r-- 1 cats archive 6891 May 5 2010 ReadMe
-rw-r--r-- 1 cats archive 1009 May 5 2010 +footg5.gif
-rw-r--r-- 1 cats archive 2274 May 5 2010 +footg8.gif
-r--r--r-- 1 cats archive 9488 Dec 3 2009 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 1766 May 5 2010 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 764 Oct 27 2009 table2.v00.gz [Uncompressed]
-r--r--r-- 1 cats archive 3841 Oct 27 2009 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/MNRAS/394/795 AGB stars in Fornax dwarf spheroidal galaxy (Whitelock+, 2009)
================================================================================
Asymptotic giant branch stars in the Fornax dwarf spheroidal galaxy.
Whitelock P.A., Menzies J.W., Feast M.W., Matsunaga N., Tanabe T., Ita Y.
<Mon. Not. R. Astron. Soc., 394, 795-809 (2009)>
=2009MNRAS.394..795W
================================================================================
ADC_Keywords: Galaxies, nearby ; Stars, giant ; Photometry, infrared
Keywords: stars: AGB and post-AGB - stars: carbon - stars: late-type -
stars: variables: other - galaxies: individual: Fornax - Local Group
Abstract:
We report on a multi-epoch study of the Fornax dwarf spheroidal
galaxy, made with the Infrared Survey Facility, over an area of
about 42x42arcmin^2^. The colour-magnitude diagram shows a broad
well-populated giant branch with a tip that slopes downwards from red
to blue, as might be expected given Fornax's known range of age and
metallicity. The extensive asymptotic giant branch (AGB) includes
seven Mira variables and 10 periodic semiregular variables. Five of
the seven Miras are known to be carbon rich. Their pulsation periods
range from 215 to 470d, indicating a range of initial masses. Three of
the Fornax Miras are redder than typical Large Magellanic Cloud (LMC)
Miras of similar period, probably indicating particularly heavy
mass-loss rates. Many, but not all, of the characteristics of the AGB
are reproduced by isochrones from Marigo et al. (2008A&A...482..883M)
for a 2Gyr population with a metallicity of Z=0.0025.
Description:
Observations were made with the SIRIUS camera on the Japanese-SAAO
Infrared Survey Facility (IRSF) at Sutherland.
Observations were made at about 15 epochs spread over 3yr in the
central 4x4 grid