V* V1695 Ori , the SIMBAD biblio

V* V1695 Ori , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.26CEST21:05:20


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Title First 3 Authors
2000AJ....119.3026R viz 1852 55 Circumstellar disk candidates identified from ultraviolet excesses in the Orion nebula cluster flanking fields. REBULL L.M., HILLENBRAND L.A., STROM S.E., et al.
2001AJ....121.1676R viz 296 104 Rotation of young low-mass stars in the Orion Nebula Cluster flanking fields. REBULL L.M.
2003AJ....125.1537T viz 1458 10 Deep near-infrared observations and identifications of Chandra sources in Orion molecular clouds 2 and 3. TSUJIMOTO M., KOYAMA K., KOBAYASHI N., et al.
2006ApJ...646..297R viz 15       D               1 471 93 A correlation between Pre-Main-Sequence stellar rotation rates and IRAC excesses in Orion. REBULL L.M., STAUFFER J.R., MEGEATH S.T., et al.
2006IBVS.5721....1K viz 1754 36 The 78th name-list of variable stars. KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al.
2007ApJ...671..605C viz 15       D               1 911 75 Testing the disk regulation paradigm with Spitzer observations. II. A clear signature of star-disk interaction in NGC 2264 and the Orion Nebula Cluster. CIEZA L. and BALIBER N.
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.
2013ApJS..208...28S viz 16       D               1 597 11 A new Hα emission-line survey in the Orion Nebula Cluster. SZEGEDI-ELEK E., KUN M., REIPURTH B., et al.
2017AJ....153..188F viz 16       D               1 810 40 NGC 1980 is not a foreground population of Orion: spectroscopic survey of young stars with low extinction in Orion A. FANG M., KIM J.S., PASCUCCI I., et al.
2019ApJ...884....6M viz 17       D               1 5696 27 Runaway young stars near the Orion Nebula. McBRIDE A. and KOUNKEL M.
2021MNRAS.503.3279S viz 17       D               1 104619 56 The GALAH survey: tracing the Galactic disc with open clusters. SPINA L., TING Y.-S., DE SILVA G.M., et al.

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