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V* V2501 Ori , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST14:32:39 |
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 |
---|---|---|---|---|---|---|---|---|---|
2001AJ....121.3160C | 1250 | 288 | Near-infrared photometric variability of stars toward the Orion A molecular cloud. | CARPENTER J.M., HILLENBRAND L.A. and SKRUTSKIE M.F. | |||||
2002ApJ...574..258F | 1124 | 251 | X-ray-emitting young stars in the Orion nebula. | FEIGELSON E.D., BROOS P., GAFFNEY III J.A., et al. | |||||
2003ApJ...582..382F | 15 | D | 1 | 646 | 42 | Chandra X-ray observation of the Orion Nebula Cluster. I. Detection, identification, and determination of X-ray luminosities. | FLACCOMIO E., DAMIANI F., MICELA G., et al. | ||
2005ApJS..160..319G | O | 2038 | 330 | Chandra Orion Ultradeep Project: observations and sources lists. | GETMAN K.V., FLACCOMIO E., BROOS P.S., et al. | ||||
2005ApJS..160..353G | 15 | D | O | 457 | 135 | Membership of the Orion nebula population from the Chandra Orion Ultradeep Project. | GETMAN K.V., FEIGELSON E.D., GROSSO N., et al. | ||
2005ApJS..160..450F | 308 | 64 | Rotational modulation of X-ray emission in Orion Nebula young stars. | FLACCOMIO E., MICELA G., SCIORTINO S., et al. | |||||
2007ApJ...659..585H | 15 | D | 453 | 4 | An X-ray spectral classification algorithm with application to young stellar clusters. | HOJNACKI S.M., KASTNER J.H., MICELA G., et al. | |||
2011IBVS.5969....1K | 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 | 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. | ||
2019A&A...626A..79P | 17 | D | 1 | 1887 | ~ | Do star clusters form in a completely mass-segregated way? | PAVLIK V., KROUPA P. and SUBR L. |