RX J0520.5+0616 , the SIMBAD biblio

RX J0520.5+0616 , the SIMBAD biblio (28 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST05:50:40

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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
1996A&AS..119....7A 164 117 New weak-line T Tauri stars in Orion from the ROSAT all-sky survey. ALCALA J.M., TERRANEGRA L., WICHMANN R., et al.
1998A&A...330.1017A 27 36 On the nature of the ROSAT X-ray selected weak-line T Tauri stars in Orion. ALCALA J.M., CHAVARRIA-K. C. and TERRANEGRA L.
2000A&A...353..186A 123 54 High-resolution spectroscopy of ROSAT low-mass pre-main sequence stars in Orion. ALCALA J.M., COVINO E., TORRES G., et al.
2000MmSAI..71.1029A 6 0 Lithium and radial velocity of ROSAT weak T Tauri stars in Orion. ALCALA J.M., COVINO E., STERZIK M., et al.
2005A&A...438..769D viz 1380 87 Pre-main sequence star Proper Motion Catalogue. DUCOURANT C., TEIXEIRA R., PERIE J.-P., 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.
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.
2012A&A...542A.115B 15       D               2 128 6 Crossing the Gould Belt in the Orion vicinity. BIAZZO K., ALCALA J.M., COVINO E., et al.
2014ApJ...786...20L viz 16       D               2 33 12 Automatic classification of time-variable X-ray sources. LO K.K., FARRELL S., MURPHY T., 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.
2015A&A...580A..88E viz 16       D               2 219 21 Search for associations containing young stars (SACY). VI. Is multiplicity universal? Stellar multiplicity in the range 3-1000 au from adaptive-optics observations. ELLIOTT P., HUELAMO N., BOUY H., et al.
2015MNRAS.454..593B viz 56       D     X         2 551 376 A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhood. BELL C.P.M., MAMAJEK E.E. and NAYLOR T.
2015A&A...583A..85A viz 731       D     X         19 214 22 Reaching the boundary between stellar kinematic groups and very wide binaries. III. Sixteen new stars and eight new wide systems in the β Pictoris moving group. ALONSO-FLORIANO F.J., CABALLERO J.A., CORTES-CONTRERAS M., et al.
2006IAUS..237..442M 19 ~ New nearby young star cluster candidates within 200 pc. MAMAJEK E.E.
2016A&A...590A..13E viz 16       D               3 646 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.459.4499E 16       D               3 61 9 The crucial role of higher order multiplicity in wide binary formation: a case study using the β-Pictoris moving group. ELLIOTT P. and BAYO A.
2017A&A...600A..83M viz 219       D   O X         6 150 9 The β Pictoris association: Catalog of photometric rotational periods of low-mass members and candidate members. MESSINA S., MILLWARD M., BUCCINO A., et al.
2017MNRAS.468.1198B 463       D     X C       11 83 10 A stellar census of the nearby, young 32 Orionis group. BELL C.P.M., MURPHY S.J. and MAMAJEK E.E.
2017AJ....154...69S viz 16       D               3 237 80 All-sky Co-moving Recovery Of Nearby Young Members (ACRONYM). II. The β Pictoris Moving Group. SHKOLNIK E.L., ALLERS K.N., KRAUS A.L., et al.
2017A&A...607A...3M 16       D               2 125 3 The β Pictoris association low-mass members: Membership assessment, rotation period distribution, and dependence on multiplicity. MESSINA S., LANZAFAME A.C., MALO L., 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...856...23G viz 16       D               1 1601 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.
2019ApJ...872...17R viz 17       D               1 449 23 HAZMAT. V. The ultraviolet and X-ray evolution of K stars. RICHEY-YOWELL T., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2019MNRAS.489.2189L viz 17       D               1 616 ~ Evaluation of nearby young moving groups based on unsupervised machine learning. LEE J. and SONG I.
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.
2020ApJ...898...27S viz 43           X         1 2727 23 BAFFLES: Bayesian ages for field lower-mass stars. STANFORD-MOORE S.A., NIELSEN E.L., DE ROSA R.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.
2022AJ....164..151L 90           X         2 60 4 A Census of the 32 Ori Association with Gaia. LUHMAN K.L.

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