RX J1140.3-8321 , the SIMBAD biblio

RX J1140.3-8321 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST16:54:58


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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.
1998A&A...338..442F 57 36 Kinematics of T Tauri stars in Chamaeleon. FRINK S., ROESER S., ALCALA J.M., et al.
2000A&A...361.1143T viz 253 41 Proper motions of pre-main sequence stars in southern star-forming regions. TEIXEIRA R., DUCOURANT C., SARTORI M.J., et al.
2001AJ....122.3325K 96 30 Multiplicity of x-ray-selected T Tauri stars in Chamaeleon. KOEHLER R.
2005AJ....129.1049C viz 157 86 Evolution of cold circumstellar dust around solar-type stars. CARPENTER J.M., WOLF S., SCHREYER K., et al.
2006A&A...446..971J 49 39 Fundamental properties of pre-main sequence stars in young, southern star forming regions: metallicities. The weak-lined T-Tauri stars. JAMES D.J., MELO C., SANTOS N.C., et al.
2006A&A...460..695T viz 15       D               1889 534 Search for associations containing young stars (SACY). I. Sample and searching method. TORRES C.A.O., QUAST G.R., DA SILVA L., et al.
2006PASP..118.1690M viz 15       D               332 82 The formation and evolution of planetary systems: placing our solar system in context with Spitzer. MEYER M.R., HILLENBRAND L.A., BACKMAN D., et al.
2007A&A...467.1147G 15       D               1 142 92 Pre-main sequence spectroscopic binaries suitable for VLTI observations. GUENTHER E.W., ESPOSITO M., MUNDT R., et al.
2008A&A...480..889S 166       D     X         5 28 39 Chemical abundances in six nearby star-forming regions. Implications for galactic evolution and planet searches around very young stars. SANTOS N.C., MELO C., JAMES D.J., et al.
2008ApJS..179..423C 15       D               2 334 51 The formation and evolution of planetary systems: description of the spitzer legacy science database. CARPENTER J.M., BOUWMAN J., SILVERSTONE M.D., et al.
2009ApJS..181..197C 15       D               1 324 164 Formation and evolution of planetary systems: properties of debris dust around solar-type stars. CARPENTER J.M., BOUWMAN J., MAMAJEK E.E., et al.
2009ApJS..184..138H viz 15       D               2 20667 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.
2010A&A...517A..88W 38         O X         1 253 31 Rotational velocities of nearby young stars. WEISE P., LAUNHARDT R., SETIAWAN J., et al.
2012AcA....62...67K viz 15       D               1 2318 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 16       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.
2013AJ....146..134K viz 16       D               1 419755 301 The radial velocity experiment (RAVE): fourth data release. KORDOPATIS G., GILMORE G., STEINMETZ M., et al.
2014A&A...568A...2S 39           X         1 96 21 The Gaia-ESO Survey: Metallicity of the Chamaeleon I star-forming region. SPINA L., RANDICH S., PALLA F., et al.
2014A&A...568A..26E viz 16       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.
2016MNRAS.459.1363J 1381       D     X   F     34 42 ~ Fundamental stellar parameters for selected T-Tauri stars in the Chamaeleon and Rho Ophiuchus star-forming regions. JAMES D.J., AARNIO A.N., RICHERT A.J.W., et al.
2017AJ....153...75K viz 16       D               1 451444 394 The Radial Velocity Experiment (RAVE): fifth data release. KUNDER A., KORDOPATIS G., STEINMETZ M., et al.
2018A&A...609A.116R viz 16       D               1 143018 65 Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. RUIZ-DERN L., BABUSIAUX C., ARENOU F., et al.
2018ApJ...867...93R viz 16       D               2 345 ~ Kinematic identification of young nearby moving groups from a sample of chromospherically active stars in the RAVE catalog. RAMIREZ-PRECIADO V.G., ROMAN-ZUNIGA C.G., AGUILAR L., et al.
2019MNRAS.490.3158C viz 17       D               1 465834 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al.
2020AJ....159..166U viz 17       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.
2020MNRAS.494.2429B viz 17       D               1 240 ~ A kinematically hot population of young stars in the solar neighbourhood. BINKS A.S., JEFFRIES R.D. and WRIGHT N.J.
2020AJ....160...83S viz 17       D               1 451371 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.
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.

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