Dust properties across the CO snowline in the HD 163296 disk from ALMA and VLA observations
To characterize the mechanisms of planet formation it is crucial to investigate the properties and evolution of protoplanetary disks around young stars, where the initial conditions for the growth of planets are set. Our goal is to study grain growth in the disk of the young, intermediate mass star...
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
January 28, 2016
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| In: |
Arxiv
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| Online-Zugang: | Verlag, Volltext: http://arxiv.org/abs/1601.07542
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| Verfasserangaben: | G. Guidi, M. Tazzari, L. Testi, I. de Gregorio-Monsalvo, C.J. Chandler, L. Pérez, A. Isella, A. Natta, S. Ortolani, Th. Hennings, S. Corder, H. Linz, S. Andrews, D. Wilner, L. Ricci, J. Carpenter, A. Sargent, L. Mundy, S. Storm, N. Calvet, C. Dullemond, J. Greaves, J. Lazio, A. Deller, and W. Kwon |
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