NGC 129 24

Query : NGC 129 24

Basic data :
NGC 129 24 -- Star
Other object types: otypes_help 		* (Cl*,GEN#,...), NIR (2MASS)
ICRS coord. (ep=J2000) : 		00 30 52.1847761352 +60 13 16.858637148 (Optical) [ 0.0089 0.0093 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) : 		00 28 03.5535833748 +59 56 43.224458358 [ 0.0089 0.0093 90 ]
Gal coord. (ep=J2000) : 		120.3781840653688 -02.5483723377304 [ 0.0089 0.0093 90 ]
Proper motions mas/yr : 		-2.474 -1.366 [0.012 0.012 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz : 		V(km/s) -37.000 [~] / z(~) -0.000123 [~] / cz -37.00 [~]
   E 2000A&AS..144....1M
Parallaxes (mas): 		0.4962 [0.0125] A 2020yCat.1350....0G
Spectral type: 		B5IVn D 1992AJ....104.1132T
Fluxes (7) :
U 11.98 [~] C 1961PUSNO..17..343H
B 12.14 [~] C 1961PUSNO..17..343H
V 11.76 [~] C 1961PUSNO..17..343H
G 11.669180 [0.002765] C 2020yCat.1350....0G
J 10.854 [0.019] C 2003yCat.2246....0C
H 10.775 [0.028] C 2003yCat.2246....0C
K 10.744 [0.021] C 2003yCat.2246....0C
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1 : 500 Display criteria :

Identifiers (16) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

NGC 129 24 Cl* NGC 129 HOAG 17 2MASS J00305217+6013168 uvby98 201290024
Cl* NGC 129 SS 378 Cl* NGC 129 HOAG 117 TIC 428457962 Gaia DR2 428618670793010432
Cl* NGC 129 LF 51 GEN# +2.01290024 TYC 4015-2782-1 Gaia DR3 428618670793010432
Cl* NGC 129 HAR 181 GSC 04015-02782 UBV M 29848 Gaia DR1 428618666489169536

References (19 between 1850 and 2026) (Total 19)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Distance : 3    Plx : 3    PM : 2   

   

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Link by name to the catalogue in VizieR :

GSC 04015-02782 2MASS J00305217+6013168 TYC 4015-2782-1 uvby98 201290024 Gaia DR2 428618670793010432
Gaia DR3 428618670793010432 Gaia DR1 428618666489169536

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