2MASS J04385548-0640248 , the SIMBAD biblio

2MASS J04385548-0640248 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST14:08:35

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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
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.
2020A&A...638A...9R viz 16       D               1 2642 ~ A census of the nearby Pisces-Eridanus stellar stream. Commonalities with and disparities from the Pleiades. ROSER S. and SCHILBACH E.
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.
2021MNRAS.506..150B viz 17       D               1 588596 276 The GALAH+ survey: Third data release. BUDER S., SHARMA S., KOS J., et al.
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.
2022ApJS..262....7H viz 17       D               1 134735 19 A Blind All-sky Search for Star Clusters in Gaia EDR3: 886 Clusters within 1.2 kpc of the Sun. HE Z., WANG K., LUO Y., et al.
2022MNRAS.517.5325H viz 17       D               1 214414 23 The GALAH survey: chemical clocks. HAYDEN M.R., SHARMA S., BLAND-HAWTHORN J., et al.
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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