The Central 1000 au of a Pre-stellar Core Revealed with ALMA. II. Almost Complete Freeze-out

Pre-stellar cores represent the initial conditions in the process of star and planet formation. Their low temperatures (\(

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Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2022-02
Hauptverfasser:	Caselli, Paola, Pineda, Jaime E, Sipilä, Olli, Zhao, Bo, Redaelli, Elena, Spezzano, Silvia, Maureira, Maria José, Alves, Felipe, Bizzocchi, Luca, Bourke, Tyler L, Chacón-Tanarro, Ana, Friesen, Rachel, Galli, Daniele, Harju, Jorma, Jiménez-Serra, Izaskun, Keto, Eric, Zhi-Yun, Li, Padovani, Marco, Schmiedeke, Anika, Tafalla, Mario, Vastel, Charlotte
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrochemistry Carbon monoxide Chemical composition Continuum radiation Depletion Deuteration Dust Freezing Initial conditions Low temperature Physics - Astrophysics of Galaxies Physics - Earth and Planetary Astrophysics Physics - Solar and Stellar Astrophysics Planet formation Planetary composition Planetary mantles Planetary systems Protoplanetary disks Radiative transfer Solid phases Stellar cores
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Beschreibung
Zusammenfassung:	Pre-stellar cores represent the initial conditions in the process of star and planet formation. Their low temperatures (\(
ISSN:	2331-8422
DOI:	10.48550/arxiv.2202.13374