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J/A+A/591/A140 IPHAS-selected classical Be stars (Gkouvelis+, 2016)
The following files can be converted to FITS (extension .fit or fit.gz)
table5.dat table6.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/591/A140
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-r--r--r-- 1 cats archive 5377 Mar 13 2018 ReadMe
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-r--r--r-- 1 cats archive 18543 Jun 20 2016 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 16191 Jul 4 2016 table6.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/A+A/591/A140 IPHAS-selected classical Be stars (Gkouvelis+, 2016)
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Physical parameters of IPHAS-selected classical Be stars.
I. Determination procedure and evaluation of the results.
Gkouvelis L., Fabregat J., Zorec J., Steeghs D., Drew J.E., Raddi R.,
Wright N.J., Drake J.J.
<Astron. Astrophys. 591, A140 (2016)>
=2016A&A...591A.140G (SIMBAD/NED BibCode)
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ADC_Keywords: Stars, early-type ; Stars, Be ; Stars, distances
Keywords: stars: early-type - stars: emission-line, Be -
stars: fundamental parameters- stars: distances -
Galaxy: structure - techniques: spectroscopic
Abstract:
We present a semi-automatic procedure to obtain fundamental physical
parameters and distances of classical Be (CBe) stars, based on the
Barbier-Chalonge-Divan (BCD) spectrophotometric system. Our aim is to
apply this procedure to a large sample of CBe stars detected by the
IPHAS photometric survey, to determine their fundamental physical
parameters and to explore their suitability as galactic structure
tracers. In this paper we describe the methodology used and the
validation of the procedure by comparing our results with those
obtained from different independent astrophysical techniques for
subsamples of stars in common with other studies. We also present a
test case study of the galactic structure in the direction of the
Perseus Galactic Arm, in order to compare our results with others
recently obtained with different techniques and the same sample of
stars. We did not find any significant clustering of stars at the
expected positions of the Perseus and Outer Galactic Arms, in
agreement with previous studies in the same area that we used for
verification.
Description:
Photometric r magnitudes, HalphaEW, BCD parameters, effective
temperatures and spectral classification for the stars studied in this
work (table 5). Spectroscopic gradient, colour excess, absolute and
intrinsic magnitudes and distances for the stars studied in this work
(table 6). The parameters of stars with multiple spectra have been
measured from each individual spectrum.
They appear as multiple entries, with the same correlative number in
the ID column