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VizieR

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The 7 columns in color are computed by VizieR, and are not part of the original data.
V/125/obcat
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Photometry and Spectroscopy for Luminous Stars (Reed 2005)
Catalog of star names/identifiers, positions, and cross-references, ordered by increasing RA (18693 rows)
img(gal)
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_RAJ2000
"h:m:s"
_DEJ2000
"d:m:s"
_RAB1950
"h:m:s"
_DEB1950
"d:m:s"
_Glon
deg
_Glat
deg
ALS

Name

mag
mag
n_

RAJ2000
"h:m:s"
DEJ2000
"d:m:s"
GLON
deg
GLAT
deg
Simbad

117 15 15.200-40 20 05.0017 11 45.901-40 16 43.06347.058492 -1.071512 3992LS 3992 9.8V17 15 15.2-40 20 05 347.06 -1.07Simbad
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V/125/obmk
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Photometry and Spectroscopy for Luminous Stars (Reed 2005)
Collation of MK classifications (22885 rows)
img(gal)
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_RAJ2000
"h:m:s"
_DEJ2000
"d:m:s"
_RAB1950
"h:m:s"
_DEB1950
"d:m:s"
_Glon
deg
_Glat
deg
ALS

TC

LC

Pec

Disp

RAJ2000
"h:m:s"
DEJ2000
"d:m:s"
BibCode

Rem

117 15 15.00-40 20 05.017 11 45.70-40 16 43.0347.05812 -1.07100 3992B6IeVarious17 15 15-40 20 051992A&A...261..482L  
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V/125/obubvbet
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Photometry and Spectroscopy for Luminous Stars (Reed 2005)
Collation of UBV-beta data (37962 rows)
img(gal)
Full

_RAJ2000
"h:m:s"
_DEJ2000
"d:m:s"
_RAB1950
"h:m:s"
_DEB1950
"d:m:s"
_Glon
deg
_Glat
deg
ALS

n_

Vmag

B-V
mag
U-B
mag
Hbeta
mag
Notes

RAJ2000
"h:m:s"
DEJ2000
"d:m:s"
BibCode

Rem

117 15 15.00-40 20 05.017 11 45.70-40 16 43.0347.05812 -1.07100 3992* 9.84 1.66 0.57    17 15 15-40 20 051985A&AS...61..387K  
217 15 15.00-40 20 05.017 11 45.70-40 16 43.0347.05812 -1.07100 3992* 9.66 1.65 0.51  Emission17 15 15-40 20 052003A&A...406..673M  
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V/125/radvel
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Photometry and Spectroscopy for Luminous Stars (Reed 2005)
*Radial velocity data (1072 rows) (Note)
 
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V/125/notes
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Photometry and Spectroscopy for Luminous Stars (Reed 2005)
Remarks on individual stars (909 rows)
 
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ALS

Text

1 3992(11.7) Machado et al. (2001A&A...368L..29M) have analysed Halpha and
2 3992 Hbeta line profiles of this peculiar supergiant, concluding that it
3 3992 may be close to the LBV phase, but it is also possible that it
4 3992 could be a B[e] supergiant. Miroshnichenko et al. [Ref 852;
5 3992 2003A&A...406..673M] report high-resolution optical spectroscopy of
6 3992 this object, concluding that this system is a B+F binary with an
7 3992 orbital period of on the order of 6 months whose orbital plane is
8 3992 viewed nearly edge-on. These authors deduce a distance of
9 3992 1.5+/-0.5kpc, and suggest that this system represents an advanced
10 3992 evolutionary stage of beta Lyrae type binary.
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