NAME LDN 1630N , the SIMBAD biblio

NAME LDN 1630N , the SIMBAD biblio (14 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST11:49:28


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Title First 3 Authors
2008AJ....135..966F viz 88 37 Evidence for early circumstellar disk evolution in NGC 2068/71. FLAHERTY K.M. and MUZEROLLE J.
2009ApJ...690..496C 45           X         1 10 145 The mid-infrared extinction law in the Ophiuchus, Perseus, and Serpens molecular clouds. CHAPMAN N.L., MUNDY L.G., LAI S.-P., et al.
2009A&A...504..461F viz 3448     A D S   X C       90 439 209 Star and protoplanetary disk properties in Orion's suburbs. FANG M., VAN BOEKEL R., WANG W., et al.
2010A&A...523A..69R 38           X         1 27 23 Detectability of giant planets in protoplanetary disks by CO emission lines. REGALY Z., SANDOR Z., DULLEMOND C.P., et al.
2011A&A...525A..47R viz 38           X         1 204 42 U-band study of the accretion properties in the σ Orionis star-forming region. RIGLIACO E., NATTA A., RANDICH S., et al.
2013ApJS..207....5F viz 289       D     X C       7 1421 96 Young stellar objects in Lynds 1641: disks, accretion, and star formation history. FANG M., KIM J.S., VAN BOEKEL R., et al.
2014MNRAS.439..256E 55       D     X         2 19 21 The {dot}M-M* relation of pre-main-sequence stars: a consequence of X-ray driven disc evolution. ERCOLANO B., MAYR D., OWEN J.E., et al.
2015A&A...581A.140S viz 40           X         1 221 12 The VISTA Orion mini-survey: star formation in the Lynds 1630 North cloud. SPEZZI L., PETR-GOTZENS M.G., ALCALA J.M., et al.
2016MNRAS.458.3479M viz 19       D               1 27 94 An all-sky support vector machine selection of WISE YSO candidates. MARTON G., TOTH L.V., PALADINI R., et al.
2018MNRAS.477..298G viz 798       D     X         20 53 6 Young star clusters in nearby molecular clouds. GETMAN K.V., KUHN M.A., FEIGELSON E.D., et al.
2021A&A...650A.157G viz 17       D               1 81 9 Dispersal timescale of protoplanetary disks in the low-metallicity young cluster Dolidze 25. GUARCELLO M.G., BIAZZO K., DRAKE J.J., et al.
2022ApJ...939L..10P 18       D               1 68 10 Most Planets Might Have More than 5 Myr of Time to Form. PFALZNER S., DEHGHANI S. and MICHEL A.
2023MNRAS.520.4646K 140           X         3 30 ~ A low-mass hub-filament with double centre revealed in NGC 2071-North. KONYVES V., WARD-THOMPSON D., SHIMAJIRI Y., et al.
2023ApJ...957...94Y 93           X         2 23 ~ TRAO Survey of Nearby Filamentary Molecular Clouds, the Universal Nursery of Stars (TRAO-FUNS). III. Filaments and Dense Cores in the NGC 2068 and NGC 2071 Regions of Orion B. YOO H., LEE C.W., CHUNG E.J., et al.

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