Imaging the Key Stages of Planet Formation

Imaging the Key Stages of Planet Formation

In this white paper, we explore how higher angular resolution beyond ALMA and 8m-class telescopes can extend our understanding of the key stages of planet formation, to resolve accreting circumplanetary disks themselves, and to watch planets forming in situ for the nearest star-forming regions.

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Bibliographische Detailangaben
Veröffentlicht in:Bulletin - American Astronomical Society 2019-05
Hauptverfasser: Monnier, John, Rau, Gioia, Bermudez, Joel Sanchez, Ragland, Sam, Akeson, Rachel, Duchene, Gaspard, van Belle, Gerard, Norris, Ryan, Gordon, Kathryn, Defrère, Denis, Kluska, Jacques, Ridgway, Stephen, Le Bouquin, Jean-Baptiste, Anugu, Narsireddy, Scott, Nicholas, Kane, Stephen, Richardson, Noel D., Regaly, Zsolt, Zhu, Zhaohuan, Vasisht, Gautam, Stassun, Keivan G., Andrews, Sean, Lacour, Sylvestre, Weigelt, Gerd, Turner, Neal, Adams, Fred C., Gies, Douglas, Calvet, Nuria, Espaillat, Catherine, Millan-Gabet, Rafael, Gardner, Tyler, Packham, Chris, Gai, Mario, Kral, Quentin, Berger, Jean-Philippe, Linz, Hendrik, Klarmann, Lucia, Bate, Matthew, Bae, Jaehan, Lopez, Rebeca Garcia, Garufi, Antonio, Baron, Fabien, Kama, Mihkel, Wilner, David, Hartmann, Lee, Kishimoto, Makoto, Olofsson, Johan, Mcclure, Melissa, Haniff, Chris, Hoenig, Sebastian, Line, Michael, Petrov, Romain G., Smith, Michael, ten Brummelaar, Theo, de Furio, Matthew, Koutoulaki, Maria, Rinehart, Stephen, Leisawitz, David, Danchi, William, Huber, Daniel, Zhang, Ke, Pope, Benjamin, Ireland, Michael, Kraus, Stefan, Isella, Andrea, Setterholm, Benjamin, White, Russel
Format: Artikel
Sprache:eng
Schlagworte:
Astrophysics
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysic
Sciences of the Universe
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Zusammenfassung:In this white paper, we explore how higher angular resolution beyond ALMA and 8m-class telescopes can extend our understanding of the key stages of planet formation, to resolve accreting circumplanetary disks themselves, and to watch planets forming in situ for the nearest star-forming regions.
ISSN:0002-7537