Autor: |
Ziwei E. Zhang, Nami Sakai, Satoshi Ohashi, Nadia M. Murillo, Claire J. Chandler, Brian Svoboda, Cecilia Ceccarelli, Claudio Codella, Luca Cacciapuoti, Ross O’Donoghue, Serena Viti, Yuri Aikawa, Eleonora Bianchi, Paola Caselli, Steven Charnley, Tomoyuki Hanawa, Izaskun Jímenez-Serra, Hauyu Baobab Liu, Laurent Loinard, Yoko Oya, Linda Podio, Giovanni Sabatini, Charlotte Vastel, Satoshi Yamamoto |
Jazyk: |
angličtina |
Rok vydání: |
2024 |
Předmět: |
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Zdroj: |
The Astrophysical Journal, Vol 966, Iss 2, p 207 (2024) |
Druh dokumentu: |
article |
ISSN: |
1538-4357 |
DOI: |
10.3847/1538-4357/ad3921 |
Popis: |
IRAS04368+2557 in L1527 is a Class 0/I protostar with a clear disk-envelope system revealed by previous Atacama Large Millimeter/submillimeter Array (ALMA) observations. In this paper, we discuss the flared structure of this source with observed sulfur-bearing molecules included in the FAUST ALMA large program. The analyses of molecular distributions and kinematics have shown that CS, SO, and OCS trace different regions of the disk-envelope system. To evaluate the temperature across the disk, we derive rotation temperature with the two observed SO lines. The temperature profile shows a clear, flared “butterfly” structure with the higher temperature being ∼50 K and the central lower temperature region ( |
Databáze: |
Directory of Open Access Journals |
Externí odkaz: |
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