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Name
  NSV 15236  
AAVSO UID
000-BBC-359 (49 observations)  
Constellation
Cassiopeia Sequence
J2000.0
01 05 07.42 +53 59 12.1  (16.28091 +53.98668) Search nearby
B1950.0 01 02 08.63 +53 43 08.3
Proper motion
RA: -1.796 +/- 1.234 mas/yDec: -1.709 +/- 0.886 mas/ySource: Gaia DR1
Galactic coord. 124.967 -8.831
Other names

(Internal only)
2MASS J01050740+5359120 ASASSN-V J010507.36+535912.0 GSC 03668-01121
LAMOST J010507.43+535912.1 NSVS 1724407 TYC 3668-1121-1
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Variability type
ACV
Spectral type kA0hB8IVpSiCrSrEu
Mag. range
11.87 - 12.01 R1
Discoverer --
Epoch
27 Dec 2012 (HJD 2456289.00) Ephemeris
Outburst --
Period 18.78 d
Rise/eclipse dur. --
Remarks
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References
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1 Hümmerich, S.; Bernhard, K., 2022, NSV 15236 (TYC 3668-1121-1) ist ein
neuer Ap/CP2-Stern		 2022BAVSR..71...77H
2 Wozniak, P. R.; et al., 2004, Northern Sky Variability Survey: Public Data
Release		 2004AJ....127.2436W
3 AAVSO Circ No.303, 1996. --
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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 = 11.06H = 10.98K = 10.94J - K = 0.12
AllWISE W1 = 10.90W2 = 10.91W3 = 11.04W1 - W2 = -0.01
APASS-DR9 B = 12.15V = 11.57g' = 11.81r' = 11.53i' = 11.55B - V = 0.59
Images
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Supporting Documents
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1 LAMOST DR4 spectrum compared to two standard star spectra Hümmerich, Stefan 2021-11-19 17:16 UTC This figure compares the LAMOST DR4 spectrum of NSV 15236 to the B8III and B9III standard spectra from the libr18_225 library (information on this library is available at http://www.appstate.edu/~grayro/mkclass/mkclassdoc.pdf).
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Revision History
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5 Bernhard, Klaus 2023-09-29 20:35 UTC Period and epoch from 2022BAVSR..71...77H. Gaia DR3 position.
4 Hümmerich, Stefan 2021-11-19 16:46 UTC Type confirmed by LAMOST DR4 spectrum. Revised spectral type given.
3 Otero, Sebastian Alberto 2020-06-09 02:27 UTC Type, period, epoch and range from NSVS data. Gaia DR2 position.
2 Admin, VSX 2012-08-14 23:30 UTC Period from NSVS data.
1 Admin, VSX 2005-12-18 01:33 UTC Initial upload.

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