Outflows, envelopes, and disks as evolutionary indicators in Lupus young stellar objects

被引：0

作者：

Vazzano, M.M. ^{[1
]}

Fernández-López, M. ^{[1
]}

Plunkett, A. ^{[2
]}

De Gregorio-Monsalvo, I. ^{[3
]}

Santamaría-Miranda, A. ^{[3
]}

Takahashi, S. ^{[4
,5
,6
]}

Lopez, C. ^{[4
]}

机构：

[1] Instituto Argentino de Radioastronomía, (CCT-La Plata, CONICET,CICPBA), Buenos Aires,1894, Argentina

[2] National Radio Astronomy Observatory, 520 Edgemont Rd, Charlottesville,VA,22903, United States

[3] European Southern Observatory, Av. Alonso de Córdova 3107, Casilla, Santiago,19001, Chile

[4] Joint ALMA Observatory, Alonso de Córdova, Vitacura, Santiago,3107, Chile

[5] NAOJ Chile Observatory, Alonso de Córdova 3788, Oficina 61B, Vitacura, Santiago, Chile

[6] Department of Astronomical Science, School of Physical Sciences, The Graduate University for Advanced Studies, SOKENDAI, Mitaka, Tokyo,181-8588, Japan

来源：

Astronomy and Astrophysics | 2021年 / 648卷

关键词：

cA knowledgements. We are very grateful to the anonymous referees for all the comments and suggestions that helped a lot to improve this work. This paper makes use of the following ALMA data: ADS/JAO.ALMA 2016.1.01141.S; ADS/JAO.ALMA; 2011.0.00777.S; 2013.1.00879.S; 2011.0.00628.S; 2013.1.00244.S; 2015.1.00306.S; 2013.1.00474.S; 2016.1.00571.S; 2016.1.00459.S; 2016.1.01239.S; ADS/JAO.ALMA 2015.1.01510.S. ALMA is a partnership of ESO (representing its member states); NSF (USA) and NINS (Japan); together with NRC (Canada); MOST and ASIAA (Taiwan); and KASI (Republic of Korea); in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO; AUI/NRAO and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities; Inc. The authors are grateful to the visiting program to JAO and ESO that facilitated this collaborative effort. M.M.V. is funded by post-graduate scholarships from the Argentine Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET). Id.G.-M. is partially supported by MCIU-AEI (Spain) grant AYA2017-84390-C2-R (co-funded by FEDER);

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摘要：

116

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