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J/other/RMxAA/44.365 New variable stars in NGC 6366 (Arellano Ferro+, 2008)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
objects.dat *.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/other/RMxAA/44.365
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drwxr-xr-x 30 cats archive 4096 Oct 18 2022 [Up]
drwxr-xr-x 2 cats archive 4096 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 485 Dec 19 2022 .message
-r--r--r-- 1 cats archive 4436 Nov 16 2008 ReadMe
-r--r--r-- 1 cats archive 18063 Sep 4 2008 candr.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 18117 Sep 4 2008 candv.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 1001 Nov 16 2008 objects.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 1647 Sep 4 2008 rrlyrv1v.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 9855 Sep 4 2008 varr.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 9693 Sep 4 2008 varv.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/other/RMxAA/44.365 New variable stars in NGC 6366 (Arellano Ferro+, 2008)
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A new search for variable stars in the globular cluster NGC 6366.
Arellano Ferro A., Giridhar S., Rojas Lopez V., Figuera R.,
Bramich D.M., Rosenzweig P.
<Rev. Mex. Astron. Astrofis., 44, 365 (2008)>
=2008RMxAA..44..365A
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ADC_Keywords: Clusters, globular ; Stars, variable ; Photometry, CCD
Keywords: globular clusters: NGC 6366 - variable stars: RR Lyrae, SX Phe -
eclipsing binaries
Abstract:
New CCD photometry of NGC 6366 has lead to the discovery of some
variable stars. Two possible Anomalous Cepheids (or Pop II Cepheids),
three long period variables, one SX Phe and one eclipsing binary have
been found. Also a list of 10 candidate variables is reported. The
light curve of the RRab star, V1, has been decomposed into its Fourier
harmonics, and the Fourier parameters were used to estimate the star's
metallicity and distance; [Fe/H]=-0.87+/-0.14 and d=3.2+/-0.1kpc. It
is argued that V1 may not be a member of the cluster but rather a more
distant object. If this is so, an upper limit for the distance to the
cluster of 2.8+/-0.1kpc can be estimated. The P-L relationship
for SX Phe stars and the identified modes in the newly discovered SX
Phe variable, V6, allow yet another independent determination of the
distance to the cluster of d=2.7+/-0.1kpc. The M_V_-[Fe/H]
relationship for RR Lyrae stars is addressed and the case of V1 is
discussed.
Objects:
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RA (2000) DE Designation(s)
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17 27 44.3 -05 04 36 NGC 6366 = C 1725-050
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