UCAC2 30793350 , the SIMBAD biblio

UCAC2 30793350 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:34:45

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2013AJ....146..134K viz 15       D               1 419759 301 The radial velocity experiment (RAVE): fourth data release. KORDOPATIS G., GILMORE G., STEINMETZ M., et al.
2017AJ....153...75K viz 16       D               1 451448 394 The Radial Velocity Experiment (RAVE): fifth data release. KUNDER A., KORDOPATIS G., STEINMETZ M., et al.
2019A&A...622L..13M viz 16       D               1 264 78 Extended stellar systems in the solar neighborhood. II. Discovery of a nearby 120° stellar stream in Gaia DR2. MEINGAST S., ALVES J. and FURNKRANZ V.
2019AJ....158...77C viz 16       D               2 156 65 TESS reveals that the nearby Pisces-Eridanus stellar stream is only 120 Myr old. CURTIS J.L., AGUEROS M.A., MAMAJEK E.E., et al.
2020ApJ...893...67M viz 16       D               1 533 31 A relationship between stellar age and spot coverage. MORRIS B.M.
2020AJ....160...83S viz 16       D               1 451375 83 The sixth Data Release of the Radial Velocity Experiment (RAVE). II. Stellar atmospheric parameters, chemical abundances, and distances. STEINMETZ M., GUIGLION G., McMILLAN P.J., et al.
2020A&A...639A..64R viz 16       D               1 4276 26 Extended stellar systems in the solar neighborhood. IV. Meingast 1: the most massive stellar stream in the solar neighborhood. RATZENBOCK S., MEINGAST S., ALVES J., et al.
2020MNRAS.496.5176D 16       D               1 304 38 Wide binaries are rare in open clusters. DEACON N.R. and KRAUS A.L.
2022ApJ...928...70C viz 17       D               1 5007 6 Pearls on a String: Numerous Stellar Clusters Strung Along the Same Orbit. CORONADO J., FURNKRANZ V. and RIX H.-W.
2024AJ....167..210V viz 18       D               1 7289 ~ The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS. VACH S., ZHOU G., HUANG C.X., et al.

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