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Latest Details
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Name
  V0492 Sco  
AAVSO UID
000-BFK-765 (No observations)  
Constellation
Scorpius Sequence
J2000.0
17 38 45.48 -34 57 17.9  (264.68950 -34.95497) Search nearby
B1950.0 17 35 25.29 -34 55 37.8
Proper motion
RA: 4.0 +/- 6.5 mas/yDec: -2.0 +/- 6.5 mas/ySource: UCAC4
Galactic coord. 354.117 -1.936
Other names

(Internal only)
Please note that aliases shown in grey link to obsolete records.
ASAS J173846-3457.3 ASASSN-V J173845.42-345718.0 HV 7916
IOMC 7384000035 [RHI84] 8- 506  
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Variability type
SR
Spectral type M7
Mag. range
13.6 - 15.8 p
Discoverer --
Epoch
05 Aug 1935 (HJD 2428020) Ephemeris
Outburst --
Period 236: d
Rise/eclipse dur. --
Remarks
There are currently no remarks on file for this star. (Not logged in)  Add remark
References
Click reference title/citation to view in new window. Roll over index number to view submission details.
1 J. Alfonso-Garzon, A. Domingo, J.M. Mas-Hesse, A. Gimenez, 2012,
arXiv:1210.0821 [astro-ph.IM] (online info)
2012arXiv1210.0821A
2 G.Pojmanski, Acta Astronomica 52, 397, 2002. 2002AcA....52..397P
3 Catalogue of Stellar Spectral Classifications (Skiff, 2005) 1984AnTok..19..469R
4 L.Plaut, Leid Ann 21, N3, 1958. --
5 H.H.Swope, HA 90, N8, 1939. 1940AnHar..90..231S
External Links
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Location    Go   
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Catalog Data
Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.
2MASS J = 3.26H = 2.03K = 1.54J - K = 1.72
AllWISE W3 = 0.17W4 = -0.60W3 - W4 = 0.77
APASS-DR9 B = 15.11V = 13.05g' = 14.30r' = 11.49B - V = 2.06
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
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Supporting Documents
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Stellar Association Membership
 ASCC 90 Open Cluster 2012A&A...548A..97Z
Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
2 Admin, VSX 2007-04-04 09:54 UTC Position and spectral type from Brian Skiff's MKTypes.dat [http://vizier.u-strasbg.fr/viz-bin/Cat?III/233B].
1 Admin, VSX 2005-12-18 01:33 UTC Initial database population.