FAUST II. Discovery of a Secondary Outflow in IRAS 15398-3359: Variability in Outflow Direction during the Earliest Stage of Star Formation?

We have observed the very low-mass Class 0 protostar IRAS 15398-3359 at scales ranging from 50 au to 1800 au, as part of the ALMA Large Program FAUST. We uncover a linear feature, visible in H2CO, SO, and C18O line emission, which extends from the source along a direction almost perpendicular to the...

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Veröffentlicht in:arXiv.org 2021-01
Hauptverfasser: Okoda, Yuki, Oya, Yoko, Logan, Francis, Johnstone, Doug, Shu-ichiro Inutsuka, Ceccarelli, Cecilia, Codella, Claudio, Chandler, Claire, Sakai, Nami, Aikawa, Yuri, Alves, Felipe, Balucani, Nadia, Bianchi, Eleonora, Bouvier, Mathilde, Caselli, Paola, Caux, Emmanuel, Charnley, Steven, Choudhury, Spandan, De Simone, Marta, Dulieu, Francois, Durán, Aurora, Evans, Lucy, Favre, Cécile, Fedele, Davide, Feng, Siyi, Fontani, Francesco, Hama, Tetsuya, Hanawa, Tomoyuki, Herbst, Eric, Hirota, Tomoya, Imai, Muneaki, Isella, Andrea, Jímenez-Serra, Izaskun, Kahane, Claudine, Lefloch, Bertrand, Loinard, Laurent, López-Sepulcre, Ana, Maud, Luke T, Maureira, Maria Jose, Menard, Francois, Mercimek, Seyma, Miotello, Anna, Moellenbrock, George, Mori, Shoji, Murillo, Nadia M, Nakatani, Riouhei, Nomura, Hideko, Oba, Yasuhiro, O'Donoghue, Ross, Ohashi, Satoshi, Ospina-Zamudio, Juan, Pineda, Jaime, Podio, Linda, Rimola, Albert, Sakai, Takeshi, Dominique Segura Cox, Yancy, Shirley, Svoboda, Brian, Taquet, Vianney, Testi, Leonardo, Vastel, Charlotte, Viti, Serena, Watanabe, Naoki, Watanabe, Yoshimasa, Witzel, Arezu, Xue, Ci, Zhang, Yichen, Zhao, Bo, Yamamoto, Satoshi
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