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Details for Revision 3
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Name
  NY Sgr  
AAVSO UID
000-BFD-826 (No observations)  
Constellation
Sagittarius Sequence
J2000.0
18 50 34.88 -23 36 17.0  (282.64533 -23.60472) Search nearby
B1950.0 18 47 32.58 -23 39 49.9
Galactic coord. 11.595 -10.343
Other names

(Internal only)
2MASS J18503488-2336170 ASAS J185034-2336.3 CMC15 J185034.8-233617
HV 4461    
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Variability type
M
Spectral type --
Mag. range
12.4 - <16.1 V
Discoverer --
Epoch
29 Aug 2002 (HJD 2452516) Ephemeris
Outburst --
Period 209 d
Rise/eclipse dur. --
Remarks
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1 Otero, Sebastian Alberto 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
Click reference title/citation to view in new window. Roll over index number to view submission details.
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 Pojmanski, G., 2002, The All Sky Automated Survey 2002AcA....52..397P
4 C.J.van Houten, Leid Ann 20, N12, 321, 1953. 1953AnLei..20..321V
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Supporting Documents
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1 Phase plot Otero, Sebastian Alberto 2016-04-29 11:19 UTC Phase plot with ASAS-3 data disentangling NY and NX Sgr.
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Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
4 Otero, Sebastian Alberto 2023-02-21 21:08 UTC Gaia DR3 position.
3 Otero, Sebastian Alberto 2016-04-29 11:19 UTC Period, epoch and maximum magnitude from ASAS-3 data. Minimum magnitude derived from CMC15. 2MASS position.
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.