2MASS J16075475-3915446 , the SIMBAD biblio

2MASS J16075475-3915446 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST01:34:38


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Title First 3 Authors
2007ApJ...655.1095A 63 26 New low-mass stars and brown dwarfs with disks in Lupus. ALLEN P.R., LUHMAN K.L., MYERS P.C., et al.
2008ApJS..177..551M viz 15       D               172 135 The Spitzer c2d survey of large, nearby, interstellar clouds. XI. Lupus observed with IRAC and MIPS. MERIN B., JORGENSEN J., SPEZZI L., et al.
2008ApJS..179..249D viz 15       D               2 227 239 Identifying the low-luminosity population of embedded protostars in the c2d observations of clouds and cores. DUNHAM M.M., CRAPSI A., EVANS II N.J., et al.
2009ApJS..181..321E viz 15       D               1 1054 1239 The Spitzer c2d legacy results: star-formation rates and efficiencies: evolution and lifetimes. EVANS N.J., DUNHAM M.M., JORGENSEN J.K., et al.
2009A&A...500.1045C viz 15       D               1 274 21 A new population of cool stars and brown dwarfs in the Lupus clouds. COMERON F., SPEZZI L. and LOPEZ MARTI B.
2009ApJS..184...18G viz 15       D               2 2602 566 A Spitzer survey of young stellar clusters within one kiloparsec of the Sun: cluster core extraction and basic structural analysis. GUTERMUTH R.A., MEGEATH S.T., MYERS P.C., et al.
2011MNRAS.418.1194M 15       D               1 100 26 Spectroscopic properties of young stellar objects in the Lupus molecular clouds. MORTIER A., OLIVEIRA I. and VAN DISHOECK E.F.
2013ApJS..205....5H viz 16       D               1 1329 12 Populations of young stellar objects in nearby molecular clouds. HSIEH T.-H. and LAI S.-P.
2015ApJS..220...11D viz 16       D               1 2988 232 Young stellar objects in the Gould belt. DUNHAM M.M., ALLEN L.E., EVANS II N.J., et al.
2016ApJ...828...46A viz 20       D               1 111 483 ALMA survey of Lupus protoplanetary disks. I. Dust and gas masses. ANSDELL M., WILLIAMS J.P., VAN DER MAREL N., et al.
2017A&A...599A.113M 1 93 155 Lupus disks with faint CO isotopologues: low gas/dust or high carbon depletion? MIOTELLO A., VAN DISHOECK E.F., WILLIAMS J.P., et al.
2017A&A...606A..88T 43           X         1 54 113 Physical properties of dusty protoplanetary disks in Lupus: evidence for viscous evolution? TAZZARI M., TESTI L., NATTA A., et al.
2018ApJ...859...21A viz 18       D               1 107 270 ALMA survey of Lupus protoplanetary disks. II. Gas disk radii. ANSDELL M., WILLIAMS J.P., TRAPMAN L., et al.
2018ApJ...865..157A 99       D       C       3 118 104 Scaling relations associated with millimeter continuum sizes in protoplanetary disks. ANDREWS S.M., TERRELL M., TRIPATHI A., et al.
2019A&A...623A.150V 42           X         1 106 34 The ALMA Lupus protoplanetary disk survey: evidence for compact gas disks and molecular rings from CN. VAN TERWISGA S.E., VAN DISHOECK E.F., CAZZOLETTI P., et al.
2020ApJ...895..126H viz 17       D               3 177 62 The evolution of dust disk sizes from a homogeneous analysis of 1-10 Myr old stars. HENDLER N., PASCUCCI I., PINILLA P., et al.
2020AJ....160..186L viz 17       D               1 235 15 A Gaia survey for young stars associated with the Lupus clouds. LUHMAN K.L.
2021AJ....162...28V viz 17       D               1 661 47 A stellar mass dependence of structured disks: a possible link with exoplanet demographics. VAN DER MAREL N. and MULDERS G.D.
2021A&A...651A..48M viz 17       D               1 73 9 Compact disks. An explanation to faint CO emission in Lupus disks. MIOTELLO A., ROSOTTI G., ANSDELL M., 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.
2022MNRAS.511.2453P 18       D               1 817 ~ Taxonomy of protoplanetary discs observed with ALMA. PARKER R., WARD-THOMPSON D. and KIRK J.
2023ApJ...942....4X 19       D               1 74 5 Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence That Disks Can Be Optically Thick at 3 mm. XIN Z., ESPAILLAT C.C., RILINGER A.M., et al.

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