RX J1216.8-7753 , the SIMBAD biblio

RX J1216.8-7753 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:01:51

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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
1995A&AS..114..109A viz 180 159 A study of the Chamaeleon star forming region from the ROSAT all-sky survey. I. X-ray observations and optical identifications. ALCALA J.M., KRAUTTER J., SCHMITT J.H.M.M., et al.
1997A&A...319..184A viz 87 86 A study of the Chamaeleon star-forming region from the ROSAT All-Sky Survey. II. The pre-main sequence population. ALCALA J.M., KRAUTTER J., COVINO E., et al.
1997A&A...328..187C 84 145 A study of the Chamaeleon star-forming region from the ROSAT all-sky survey. III. High resolution spectroscopic study. COVINO E., ALCALA J.M., ALLAIN S., et al.
2000MmSAI..71.1021T 22 1 An atlas of high resolution spectra of ROSAT-discovered weak T-Tauri stars in Chamaeleon. TRIPICCHIO A., ALCALA J.M., COVINO E., et al.
2001AJ....122.3325K 96 30 Multiplicity of x-ray-selected T Tauri stars in Chamaeleon. KOEHLER R.
2003A&A...404..913S viz 1239 88 Formation scenarios for the young stellar associations between galactic longitudes l=280°-360°. SARTORI M.J., LEPINE J.R.D. and DIAS W.S.
2005A&A...438..769D viz 1380 87 Pre-main sequence star Proper Motion Catalogue. DUCOURANT C., TEIXEIRA R., PERIE J.-P., et al.
2006AJ....132..866R viz 15       D               1076 188 Identification of new M dwarfs in the solar neighborhood. RIAZ B., GIZIS J.E. and HARVIN J.
2006ApJ...645.1283P 116 75 The Spitzer c2d survey of weak-line T Tauri stars. I. Initial results. PADGETT D.L., CIEZA L., STAPELFELDT K.R., et al.
2009ApJS..184..138H viz 15       D               2 20623 68 XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. HAAKONSEN C.B. and RUTLEDGE R.E.
2010MNRAS.401.1151M viz 15       D               1 3443 20 The RASS-6dFGS catalogue: a sample of X-ray selected AGN from the 6dF galaxy survey. MAHONY E.K., CROOM S.M., BOYLE B.J., et al.
2010ApJ...724..835W viz 15       D               2 203 62 The Spitzer c2d survey of weak-line T Tauri stars. III. The transition from primordial disks to debris disks. WAHHAJ Z., CIEZA L., KOERNER D.W., et al.
2005yCat.3244....0G viz 15       D               2 26640 61 Catalog of Stellar Rotational Velocities GLEBOCKI R. and GNACINSKI P.
2012AcA....62...67K viz 15       D               1 2326 121 ASAS photometry of ROSAT sources. I. Periodic variable stars coincident with bright sources from the ROSAT All Sky Survey. KIRAGA M.
2013A&A...551A..46L viz 15       D   O           3 248 21 Proper motions of young stars in Chamaeleon. I. A virtual observatory study of spectroscopically confirmed members. LOPEZ MARTI B., JIMENEZ-ESTEBAN F., BAYO A., et al.
2013MNRAS.435.1325M viz 246       D     X         7 100 50 Re-examining the membership and origin of the ε Cha association. MURPHY S.J., LAWSON W.A. and BESSELL M.S.
2014A&A...568A..26E viz 15       D               1 270 46 Search for associations containing young stars (SACY). V. Is multiplicity universal? Tight multiple systems. ELLIOTT P., BAYO A., MELO C.H.F., et al.
2016A&A...590A..13E viz 16       D               2 646 29 Search for associations containing young stars (SACY). VII. New stellar and substellar candidate members in the young associations. ELLIOTT P., BAYO A., MELO C.H.F., et al.
2017AJ....154..195B viz 16       D               3 59 2 New binaries in the ε Cha association. BRICENO C. and TOKOVININ A.
2018ApJ...856...23G viz 16       D               1 1600 367 BANYAN. XI. The BANYAN Σ multivariate Bayesian algorithm to identify members of young associations with 150 pc. GAGNE J., MAMAJEK E.E., MALO L., et al.
2018ApJ...867..151D viz 16       D               1 389 80 Distances and kinematics of Gould Belt star-forming regions with Gaia DR2 results. DZIB S.A., LOINARD L., ORTIZ-LEON G.N., et al.
2018A&A...620A.172Z viz 16       D               1 127610 99 3D mapping of young stars in the solar neighbourhood with Gaia DR2. ZARI E., HASHEMI H., BROWN A.G.A., et al.
2019ApJ...877...60B viz 16       D               3 658 26 The elusive majority of young moving groups. I. Young binaries and lithium-rich stars in the solar neighborhood. BOWLER B.P., HINKLEY S., ZIEGLER C., et al.
2020AJ....159..166U viz 16       D               1 615 26 Analysis of membership probability in nearby young moving groups with Gaia DR2. UJJWAL K., KARTHA S.S., MATHEW B., et al.
2021A&A...645A..30Z viz 17       D               1 431 20 Search for associations containing young stars (SACY). VIII. An updated census of spectroscopic binary systems exhibiting hints of non-universal multiplicity among their associations. ZUNIGA-FERNANDEZ S., BAYO A., ELLIOTT P., et al.
2021AJ....161...87D viz 17       D               4 81 ~ Gaia-based isochronal, kinematic, and spatial analysis of the ε Cha Association. DICKSON-VANDERVELDE D.A., WILSON E.C. and KASTNER J.H.
2022MNRAS.511.6179L viz 17       D               1 2244 3 Low-mass members of nearby young stellar moving groups from Gaia EDR3. LEE J., SONG I. and MURPHY S.J.
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.
2023ApJS..265...12Q viz 17       D               1 58898 5 Hunting for Neighboring Open Clusters with Gaia DR3: 101 New Open Clusters within 500 pc. QIN S., ZHONG J., TANG T., et al.
2023A&A...674A..21M viz 17       D               1 11510 8 Gaia Data Release 3 Validating the classification of variable young stellar object candidates. MARTON G., ABRAHAM P., RIMOLDINI L., et al.
2023A&A...677A..59R viz 17       D               1 13197 ~ Significance mode analysis (SigMA) for hierarchical structures An application to the Sco-Cen OB association. RATZENBOCK S., GROSSSCHEDL J.E., MOLLER T., 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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