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Name
  NSV 14402  
AAVSO UID
000-BDC-629 (1764 observations)  
Constellation
Cassiopeia Sequence
J2000.0
23 02 41.11 +59 33 28.0  (345.67129 +59.55778) Search nearby
B1950.0 23 00 35.87 +59 17 17.4
Proper motion
RA: -0.200 +/- 0.513 mas/yDec: 14.125 +/- 0.462 mas/ySource: Gaia DR1
Galactic coord. 109.546 -0.457
Other names

(Internal only)
AAVSO 2258+59D AFGL 3016 BD+58 2534
HD 217849 IOMC 3997000063 IRAS 23005+5917
RAFGL 3016 SAO 35094  
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Variability type
LB:
Spectral type K5III
Mag. range
7.54 (0.1:) V
Discoverer --
Epoch
--
Outburst --
Period --
Rise/eclipse dur. --
Remarks
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References
Click reference title/citation to view in new window. Roll over index number to view submission details.
1 J. Alfonso-Garzon, A. Domingo, J.M. Mas-Hesse, A. Gimenez, 2012,
arXiv:1210.0821 [astro-ph.IM] (online info)
2012arXiv1210.0821A
2 E.S.Brodskaya, Izv Crimean Obs 14, 1955. --
3 Malmquist, K. G.; Schalen, C.; Westerlund, B., 1954, A Spectrophotometric
Survey of Stars Along the Milky Way: Part I. Galactic Longitudes 60° -80°
1954UppAn...4a...1M
External Links
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Location    Go   
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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 = 4.80H = 3.86K = 3.66J - K = 1.14
AllWISE W1 = 3.82W2 = 3.67W3 = 3.85W4 = 3.77W1 - W2 = 0.15W3 - W4 = 0.09
APASS-DR9
SDSS-DR12 u = 13.09g = 12.54r = 10.08i = 12.84z = 10.62u - g = 0.55r - i = -2.75
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 23 02 41.11 +59 33 28.0 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
2 Otero, Sebastian Alberto 2021-05-13 21:59 UTC Spectral type from 1954UppAn...4a...1M. Gaia EDR3 position. Mean magnitude derived from Tycho-2 and Gaia EDR3. Amplitude from AAVSO and INTEGRAL-OMC data.
1 Admin, VSX 2005-12-18 01:33 UTC Preserved original object data.