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Name |
NSV 23451 |
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AAVSO UID |
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Constellation |
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J2000.0 |
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B1950.0 |
17 39 01.72 -24 59 10.9 |
Galactic coord. |
2.936 +2.723 |
Other names

(Internal only)
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OGLE BLG334.2.141952 |
OGLE-BLG-LPV-018679 |
OGLE-III BLG334.2.141952 |
OGLE-IV BLG714.19.44905 |
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Variability type |
M |
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Spectral type |
-- |
Mag. range |
14.203 (3.064) Ic |
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Discoverer |
-- |
Epoch |
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Outburst |
-- |
Period |
166.62 d |
Rise/eclipse dur. |
-- |
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Remarks
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Some references may be clicked to view in new window. Roll over index number to view submission details.
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References
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Click reference title/citation to view in new window. Roll over index number to view submission details.
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1 |
Iwanek, P.; et al., 2022, The OGLE Collection of Variable Stars: Nearly 66,000 Mira Stars in the Milky Way |
2022ApJS..260...46I |
2 |
I. Soszynski, A. Udalski, M.K. Szymanski et al., 2013, Acta Astronomica 63, 21 (online V data) |
2013arXiv1304.2787S |
3 |
I. Soszynski, A. Udalski, M.K. Szymanski et al., 2013, Acta Astronomica 63, 21 (online I data) |
2013arXiv1304.2787S |
4 |
I. Soszynski, A. Udalski, M.K. Szymanski et al., 2013, Acta Astronomica 63, 21 (Chart) |
2013arXiv1304.2787S |
5 |
I. Soszynski, A. Udalski, M.K. Szymanski et al., 2013, Acta Astronomica 63, 21 |
2013arXiv1304.2787S |
6 |
Soszynski, I.; et al., 2013, The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. XV. Long-Period Variables in the Galactic Bulge |
2013AcA....63...21S |
7 |
A.Terzan, E.Gosset, AsAp Suppl 90, No.3, 451, 1991. |
1991A&AS...90..451T |
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External Links
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Location
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Catalog Data
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Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.
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2MASS
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J = 10.35 | H = 9.07 | K = 8.32 | J - K = 2.03 |
AllWISE
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W1 = 8.19 | W2 = 7.84 | W3 = 6.82 | W4 = 6.15 | W1 - W2 = 0.35 | W3 - W4 = 0.67 |
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Images
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Please review Digitized Sky Survey Acknowledgment and Copyright.
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Supporting Documents
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Revision History
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Currently approved revision is checked. Click revision number to view details of that revision.
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