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Latest Details
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Name |
NY Sgr |
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AAVSO UID |
000-BFD-826 (No observations) |
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Constellation |
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J2000.0 |
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B1950.0 |
18 47 32.59 -23 39 50.0 |
Galactic coord. |
11.595 -10.343 |
Other names

(Internal only)
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2MASS J18503488-2336170 |
ASAS J185034-2336.3 |
CMC15 J185034.8-233617 |
HV 4461 |
OGLE-BLG-LPV-266076 |
OGLE-IV BLG406.04.3 |
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Variability type |
M |
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Spectral type |
-- |
Mag. range |
12.4 - <16.1 V |
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Discoverer |
-- |
Epoch |
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Outburst |
-- |
Period |
209 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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1 |
Otero, Sebastian Alberto
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J-K= 1.43. Two miras 11" apart, NY and NX Sgr. NY Sgr is the fainter one as it has been shown in the original reports (13.7 - 16.5 p in 1928BHarO.858...13W) and the currently available photometry (V= 12.4 - <16.1). In 1953AnLei..20..321Vm van Houten only studies the brighter variable (12.7 - <14.1 p, P= 159 d. and 12.5 - 16.0 p in 1928BHarO.858...13W, V= 11.3 - <16.1 in the currently available photometry) and erroneously identifies it as NY Sgr instead of NX Sgr. The ASAS-3 light curve includes light from both stars and is also contaminated by 2MASS J18503492-2336226 (V= 15.2; sep. 6") and 2MASS J8503307-2336208 (V= 13.8; sep. 25"). Range has been corrected. |
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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 |
Pojmanski, G., 2002, The All Sky Automated Survey |
2002AcA....52..397P |
3 |
C.J.van Houten, Leid Ann 20, N12, 321, 1953. |
1953AnLei..20..321V |
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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 = 9.07 | H = 8.14 | K = 7.65 | J - K = 1.43 |
AllWISE
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W1 = 7.39 | W2 = 6.96 | W3 = 6.22 | W4 = 5.16 | W1 - W2 = 0.44 | W3 - W4 = 1.06 |
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Images
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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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4 |
Otero, Sebastian Alberto
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2023-02-21 21:08 UTC |
Gaia DR3 position. |
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3 |
Otero, Sebastian Alberto
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2016-04-29 11:19 UTC |
Period, epoch and maximum magnitude from ASAS-3 data. Minimum magnitude derived from CMC15. 2MASS position. |
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2 |
Admin, VSX
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2010-01-05 04:43 UTC |
Position updated from the GCVS version of November 2009. |
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1 |
Admin, VSX
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2005-12-18 01:33 UTC |
Initial upload. |
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