PM J11529+3554 , the SIMBAD biblio

PM J11529+3554 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST15:39:31


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Title First 3 Authors
2003A&A...406..535Z viz 15       D               1 10290 80 The Hamburg/RASS Catalogue of optical identifications. Northern high-galactic latitude ROSAT Bright Source Catalogue X-ray sources. ZICKGRAF F.-J., ENGELS D., HAGEN H.-J., et al.
2009ApJS..184..138H viz 15       D               2 20665 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.
2011AJ....141..166H viz 15       D               1 2142 129 A photometric variability survey of field K and M dwarf stars with HATNet. HARTMAN J.D., BAKOS G.A., NOYES R.W., et al.
2011AJ....142..138L viz 15       D               1 8897 232 An all-sky catalog of bright M dwarfs. LEPINE S. and GAIDOS E.
2011ApJ...743...48W viz 15       D               1 800 589 The stellar-activity-rotation relationship and the evolution of stellar dynamos. WRIGHT N.J., DRAKE J.J., MAMAJEK E.E., et al.
2015ApJ...798...41A viz 16       D               1 802 19 The near-ultraviolet luminosity function of young, early M-type dwarf stars. ANSDELL M., GAIDOS E., MANN A.W., et al.
2020MNRAS.492.5844R 187       D       C F     5 81 ~ First results from MFOSC-P: low-resolution optical spectroscopy of a sample of M dwarfs within 100 parsecs. RAJPUROHIT A.S., KUMAR V., SRIVASTAVA M.K., et al.
2020A&A...638A..20M viz 17       D               1 314 44 Relation of X-ray activity and rotation in M dwarfs and predicted time-evolution of the X-ray luminosity. MAGAUDDA E., STELZER B., COVEY K.R., et al.
2023MNRAS.524.6085K 19       D               2 83 ~ Exploring the short-term variability of H α and H β emissions in a sample of M dwarfs. KUMAR V., RAJPUROHIT A.S., SRIVASTAVA M.K., et al.
2024ApJ...960...62E 20       D               1 258 ~ Living with a Red Dwarf: X-Ray, UV, and Ca II Activity-Age Relationships of M Dwarfs. ENGLE S.G.

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