2MASS J01241868+4308315, BD+42 293, HD 8441, HIP 6560, TYC 2825-2536-1, SAO 37177
Database references
SIMBAD
data
HN Andromedae (often abbreviated to HN And) is a variable star in the constellation Andromeda. Its apparent visual magnitude varies between 6.67 and 6.76[3] in a cycle of 69.51 days.[10] It is classified as an α2 Canum Venaticorum variable.[3]
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^ abcdefBrown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
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HNAndromedae (often abbreviated to HN And) is a variable star in the constellation Andromeda. Its apparent visual magnitude varies between 6.67 and 6...
Exoplanets 14 Andromedae b κ Andromedae b υ Andromedae b c d Gliese 15 Ab c HD 13931 b HD 16175 b HAT-P-6b HAT-P-32b WASP-1b WASP-33b Qatar-4b Qatar-5b...
; Kirkpatrick, J. Davy; Roellig, Thomas L.; Allers, K. N. (August 2008). "HN Peg B: A Test of Models of the L to T Dwarf Transition". The Astrophysical...
Ridgway, S. T. (2000), "Identification of SH v=1 Ro-vibrational Lines in R Andromedae", The Astrophysical Journal, 528 (1): L33–L36, arXiv:astro-ph/9911080...
1.33 ± 0.03 6412.830+102.682 −110.120 Also known as HD 147506 c Beta Andromedae b 28.26+2.05 −2.17 663.87+4.61 −4.31 2.03 ± 0.01 radial vel. 199.36184 ± 9...