Wolf 1120

Query : Wolf 1120

Basic data :
Wolf 1120 -- High Proper Motion Star
Other object types: otypes_help 		* (ASCC,UCAC4,...), PM* (2016ApJS,NLTT,...), NIR (2MASS), MIR (WISEA)
ICRS coord. (ep=J2000) : 		19 54 17.2560847728 +53 46 42.320176464 (Optical) [ 0.0120 0.0110 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) : 		19 53 03.6110715399 +53 38 55.400837972 [ 0.0120 0.0110 90 ]
Gal coord. (ep=J2000) : 		087.2094775021022 +13.0287646020684 [ 0.0120 0.0110 90 ]
Proper motions mas/yr : 		-18.994 -199.730 [0.016 0.015 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz : 		V(km/s) 1.41 [0.52] / z(spectroscopic) 0.000005 [0.000002] / cz 1.41 [0.52]
   (Opt) A 2018yCat.1345....0G
Parallaxes (mas): 		20.1743 [0.0122] A 2020yCat.1350....0G
Fluxes (9) :
B 14.63 [~] D 2001KFNT...17e.409K
R 12.712 [0.09] D 2012yCat.1322....0Z
G 12.306450 [0.002791] C 2020yCat.1350....0G
J 9.938 [0.027] C 2003yCat.2246....0C
H 9.333 [0.031] C 2003yCat.2246....0C
K 9.092 [0.019] C 2003yCat.2246....0C
g 13.809 [0.01] D 2012yCat.1322....0Z
r 12.566 [0.01] D 2012yCat.1322....0Z
i 11.635 [0.01] D 2012yCat.1322....0Z
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1 : 13 Display criteria :

Identifiers (12) :
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NLTT 48435 2MASS J19541725+5346422 UCAC4 719-066318 Wolf 1120
ASCC 272135 PM J19542+5346 USNO-B1.0 1437-00302298 Gaia DR2 2137629515554250752
LSPM J1954+5346 TIC 264393379 WISEA J195417.23+534640.2 Gaia DR3 2137629515554250752

References (10 between 1850 and 2026) (Total 10)
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

Velocities : 1    Distance : 2    Plx : 2    PM : 4   

   

External archives :

Link by name to the catalogue in VizieR :

NLTT 48435 LSPM J1954+5346 2MASS J19541725+5346422 UCAC4 719-066318 USNO-B1.0 1437-00302298
WISEA J195417.23+534640.2 Gaia DR2 2137629515554250752 Gaia DR3 2137629515554250752

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