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Details for Revision 3
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Name
  V0343 Ser  
AAVSO UID
000-BCX-242 (24 observations)  
Constellation
Serpens Sequence
J2000.0
18 12 22.15 -11 40 07.1  (273.09229 -11.66864) Search nearby
B1950.0 18 09 34.63 -11 40 55.1
Galactic coord. 18.090 +3.190
Other names

(Internal only)
Please note that aliases shown in grey link to obsolete records.
2MASS J18122215-1140070 AAVSO 1806-11 AS 289
ASAS J181222-1140.1 GSC 05684-00522 Hen 3-1627
IRAS 18095-1140 NSV 24326 SS73 143
TmzV17    
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Variability type
ZAND+SRA
Spectral type B+M3-M4IIIe
Mag. range
11.57 - 13.62 V
Discoverer --
Epoch
30 Aug 2003 (HJD 2452882) Ephemeris
Outburst --
Period 491 d
Rise/eclipse dur. --
Remarks
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1 Otero, Sebastian Alberto Spectroscopic orbital period 450.5 d. (2001AJ....121.2219F).
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References
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1 M. Gromadzki, J. Mikolajewska, I. Soszynski, 2013, arXiv:1312.6063
[astro-ph.SR]		 2013arXiv1312.6063G
2 G.Pojmanski, Acta Astronomica 52, 397, 2002. 2002AcA....52..397P
3 Fekel, F. C., et al., 2001, Infrared Spectroscopy of Symbiotic Stars. III.
First Orbits for Three S-Type Systems		 2001AJ....121.2219F
4 Munari, U., et al., 1992, UBVRI-JHKL photometric catalogue of symbiotic
stars		 1992A&AS...93..383M
5 Munari, U., et al., 1992, UBVRI-JHKL photometric catalogue of symbiotic
stars		 1992A&AS...93..383M
6 BAA VSS Circ No.72, 27, 1991. --
7 D.A.Allen, Proc ASA 5, No.3, 369, 1984. 1984PASAu...5..369A
8 K.Takamizawa, M.Wakuda, T.Kato, VSNET No.1457, 1998
(http://www.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet/maillist.html).		 --
External Links
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Supporting Documents
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Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
4 Admin, VSX 2013-12-27 05:49 UTC Update from [2013arXiv1312.6063G].
3 Otero, Sebastian Alberto 2013-03-04 23:46 UTC Period, epoch and maximum magnitude from ASAS-3 data. Minimum magnitude from 1992A&AS...93..383M. Orbital period from 2001AJ....121.2219F.
2 Admin, VSX 2010-01-05 04:43 UTC Position updated from the GCVS version of November 2009.
1 Admin, VSX 2005-12-18 01:33 UTC Initial upload.

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