Molecules with ALMA at Planet-forming Scales. XX. The Massive Disk around GM Aurigae

Gas mass remains one of the most difficult protoplanetary disk properties to constrain. With much of the protoplanetary disk too cold for the main gas constituent, H 2 , to emit, alternative tracers such as dust, CO, or the H 2 isotopologue HD are used. However, relying on disk mass measurements fro...

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Veröffentlicht in:	The Astrophysical Journal Supplement Series 2021-11, Vol.257 (1), p.20
Hauptverfasser:	Schwarz, Kamber R., Calahan, Jenny K., Zhang, Ke, Alarcón, Felipe, Aikawa, Yuri, Andrews, Sean M., Bae, Jaehan, Bergin, Edwin A., Booth, Alice S., Bosman, Arthur D., Cataldi, Gianni, Cleeves, L. Ilsedore, Czekala, Ian, Huang, Jane, Ilee, John D., Law, Charles J., Le Gal, Romane, Liu, Yao, Long, Feng, Loomis, Ryan A., Macías, Enrique, McClure, Melissa, Ménard, François, Öberg, Karin I., Teague, Richard, van Dishoeck, Ewine, Walsh, Catherine, Wilner, David J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrochemistry Carbon monoxide Dust Planet formation Planets Protoplanetary disk Protoplanetary disks Radio telescopes Reduction Sciences of the Universe Spatial resolution Temperature structure Tracers
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