V* V2172 Ori , the SIMBAD biblio

V* V2172 Ori , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST16:44:42

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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
1995AJ....109..709A viz 1723 62 A 2.2 mu.m imaging survey of the Orion A molecular cloud. ALI B. and DEPOY D.L.
2001AJ....121.3160C viz 1250 288 Near-infrared photometric variability of stars toward the Orion A molecular cloud. CARPENTER J.M., HILLENBRAND L.A. and SKRUTSKIE M.F.
2002A&A...396..513H viz 1564 244 Stellar rotation and variability in the Orion Nebula Cluster. HERBST W., BAILER-JONES C.A.L., MUNDT R., et al.
2009ApJS..183..261D viz 15       D               1 2645 47 A multi-color optical survey of the Orion nebula cluster. I. The catalog. DA RIO N., ROBBERTO M., SODERBLOM D.R., et al.
2009A&A...502..883R viz 15       D               1 2914 51 Rotational studies in the Orion nebula cluster: from solar mass stars to brown dwarfs. RODRIGUEZ-LEDESMA M.V., MUNDT R. and EISLOEFFEL J.
2011IBVS.5969....1K viz 15       D               1 2040 27 The 80th name-list of variable stars. Part I - RA 0h to 6h. KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al.
2011ApJ...733...50M viz 15       D               1 2085 188 YSOVAR: the first sensitive, wide-area, mid-infrared photometric monitoring of the Orion Nebula Cluster. MORALES-CALDERON M., STAUFFER J.R., HILLENBRAND L.A., et al.
2012ApJ...748...14D viz 15       D               1 1755 122 The initial mass function of the Orion Nebula Cluster across the H-burning limit. DA RIO N., ROBBERTO M., HILLENBRAND L.A., et al.
2012ApJ...755..154M viz 15       D               1 715 76 Hubble Space Telescope measures of mass accretion rates in the Orion Nebula Cluster. MANARA C.F., ROBBERTO M., DA RIO N., et al.
2012AJ....144..192M viz 15       D               1 3517 337 The Spitzer Space Telescope survey of the Orion A and B molecular clouds. I. A census of dusty young stellar objects and a study of their mid-infrared variability. MEGEATH S.T., GUTERMUTH R., MUZEROLLE J., et al.
2015ApJ...807...27C viz 16       D               7 4784 27 IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. COTTAAR M., COVEY K.R., FOSTER J.B., et al.
2016ApJ...818...59D viz 16       D               1 2715 93 IN-SYNC. IV. The young stellar population in the Orion A molecular cloud. DA RIO N., TAN J.C., COVEY K.R., et al.
2016ApJS..226....8K viz 16       D               1 347 12 The Spitzer infrared spectrograph survey of protoplanetary disks in Orion A. I. Disk properties. KIM K.H., WATSON D.M., MANOJ P., et al.
2018AJ....156...84K viz 16       D               1 9041 228 The APOGEE-2 survey of the Orion star-forming Complex. II. Six-dimensional structure. KOUNKEL M., COVEY K., SUAREZ G., et al.
2018ApJ...869...72Y viz 16       D               1 1662 2 IN-SYNC. VIII. Primordial disk frequencies in NGC 1333, IC 348, and the Orion A molecular cloud. YAO Y., MEYER M.R., COVEY K.R., et al.
2019A&A...622A.149G viz 17       D               1 3134 39 VISION - Vienna survey in Orion. III. Young stellar objects in Orion A. GROSSSCHEDL J.E., ALVES J., TEIXEIRA P.S., et al.
2019AJ....157..196K viz 17       D               1 12851 76 Close companions around young stars. KOUNKEL M., COVEY K., MOE M., et al.
2019ApJ...884....6M viz 17       D               1 5696 27 Runaway young stars near the Orion Nebula. McBRIDE A. and KOUNKEL M.
2019ApJ...886...95D 17       D               1 108 17 A search for intermediate-separation low-mass binaries in the Orion Nebula Cluster. DE FURIO M., REITER M., MEYER M.R., et al.
2021ApJ...920..132P viz 17       D               1 5441 33 Quantifying variability of young stellar objects in the mid-infrared over 6 years with the Near-Earth Object Wide-field Infrared Survey Explorer. PARK W., LEE J.-E., CONTRERAS PENA C., et al.
2021ApJ...923..177S viz 17       D               1 9744 13 Stellar rotation of T Tauri stars in the Orion Star-forming Complex. SERNA J., HERNANDEZ J., KOUNKEL M., et al.

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