Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): The SPHERE view of the Orion star-forming region

被引：0

作者：

Valegård, P.-G. ^{[1
]}

Ginski, C. ^{[2
]}

Derkink, A. ^{[1
]}

Garufi, A. ^{[3
]}

Dominik, C. ^{[1
]}

Ribas, Á. ^{[4
]}

Williams, J.P. ^{[5
]}

Benisty, M. ^{[6
]}

Birnstiel, T. ^{[7
,8
]}

Facchini, S. ^{[9
]}

Columba, G. ^{[10
,11
]}

Hogerheijde, M. ^{[1
,12
]}

Van Holstein, R.G. ^{[13
]}

Huang, J. ^{[14
]}

Kenworthy, M. ^{[12
]}

Manara, C.F. ^{[15
]}

Pinilla, P. ^{[16
,17
]}

Rab, Ch. ^{[7
,18
]}

Sulaiman, R. ^{[19
]}

Zurlo, A. ^{[20
,21
]}

机构：

[1] Anton Pannekoek Institute for Astronomy (API), University of Amsterdam, Science Park 904, Amsterdam,1098 XH, Netherlands

[2] School of Natural Sciences, Center for Astronomy, University of Galway, Galway,H91 CF50, Ireland

[3] Inaf, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, Firenze,50125, Italy

[4] Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge,CB3 0HA, United Kingdom

[5] Institute for Astronomy, University of Hawaii, Honolulu,HI,96822, United States

[6] University of Grenoble Alps, Cnrs, Ipag, Grenoble,38000, France

[7] University Observatory, Faculty of Physics, Ludwig-Maximilians-Universität München, Scheinerstr. 1, Munich,81679, Germany

[8] Exzellenzcluster Origins, Boltzmannstr. 2, Garching,85748, Germany

[9] Dipartimento di Fisica, Università Degli Studi di Milano, Via Celoria 16, Milano,20133, Italy

[10] Department of Physics and Astronomy Galileo Galilei, University of Padova, Vicolo dell'Osservatorio 3, Padova,35122, Italy

[11] Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova,35122, Italy

[12] Leiden Observatory, Leiden University, Niels Bohrweg 2, Leiden,2333 CA, Netherlands

[13] European Southern Observatory, Alonso de Córdova 3107, Casilla 19001, Vitacura, Santiago, Chile

[14] Department of Astronomy, Columbia University, 538 W. 120th Street, Pupin Hall, New York,NY,10027, United States

[15] European Southern Observatory, Karl-Schwarzschild-Strasse 2, Garching bei München,85748, Germany

[16] Max-Planck-Institut für Astronomie, Königstuhl 17, Heidelberg,69117, Germany

[17] Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey,RH5 6NT, United Kingdom

[18] Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse 1, Garching,85748, Germany

[19] Department of Physics, American University of Beirut, PO Box 110236, Riad El-Solh, Beirut,11097 2020, Lebanon

[20] Instituto de Estudios Astrofísicos, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago, Chile

[21] Escuela de Ingeniería Industrial, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago, Chile

来源：

Astronomy and Astrophysics | 1600年 / 685卷

关键词：

129;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Journal article (JA)

引用

共 39 条

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ASTRONOMISCHE NACHRICHTEN, 2009, 330 (05) : 482 - 492
[32] A multi-wavelength study of pre-main sequence stars in the Taurus-Auriga star-forming region
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[33] Deep imaging surveys of star-forming clouds. IV. The meek and the mighty: Outflows from young stars in Chamaeleon I
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Luhman, Kevin L.
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ASTRONOMICAL JOURNAL, 2006, 132 (05): : 1923 - 1937
[34] An unusual abundance of T Tauri stars? NIR study of the southern high-mass star-forming region RCW 34
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STAR CLUSTERS: BASIC GALACTIC BUILDING BLOCKS THROUGHOUT TIME AND SPACE, 2010, (266): : 384 - 384
[35] A systematic study of X-ray flares from low-mass young stellar objects in the ρ Ophiuchi star-forming region with Chandra
Imanishi, K
Nakajima, H
Tsujimoto, M
Koyama, K
Tsuboi, Y
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2003, 55 (03) : 653 - 681
[36] Anatomy of the massive star-forming region S106 The [O I] 63 μm line observed with GREAT/SOFIA as a versatile diagnostic tool for the evolution of massive stars
Schneider, N.
Roellig, M.
Simon, R.
Wiesemeyer, H.
Gusdorf, A.
Stutzki, J.
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Richter, H.
ASTRONOMY & ASTROPHYSICS, 2018, 617
[37] Rotational velocities for B0-B3 stars in seven young clusters: Further study of the relationship between rotation speed and density in star-forming regions
Wolff, S. C.
Strom, S. E.
Dror, D.
Venn, K.
ASTRONOMICAL JOURNAL, 2007, 133 (03): : 1092 - 1103
[38] The sharpest view on the high-mass star-forming region S255IR Near infrared adaptive optics imaging of the outbursting source NIRS3
Fedriani, R.
Garatti, A.
Cesaroni, R.
Tan, J. C.
Stecklum, B.
Moscadelli, L.
Koutoulaki, M.
Cosentino, G.
Whittle, M.
ASTRONOMY & ASTROPHYSICS, 2023, 676
[39] Rotational velocities for early-type stars in the young large magellanic cloud cluster R136: Further study of the relationship between rotation speed and density in star-forming regions
Wolff, S. C.
Strom, S. E.
Cunha, K.
Daflon, S.
Olsen, K.
Dror, D.
ASTRONOMICAL JOURNAL, 2008, 136 (03): : 1049 - 1060

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