Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Frankie Encalada"'
Autor:
Erin G. Cox, Giles Novak, Sarah I. Sadavoy, Leslie W. Looney, Dennis Lee, Marc Berthoud, Tyler L. Bourke, Simon Coudé, Frankie Encalada, Laura M. Fissel, Rachel Harrison, Martin Houde, Zhi-Yun Li, Philip C. Myers, Kate Pattle, Fabio P. Santos, Ian W. Stephens, Hailin Wang, Sebastian Wolf
We present H-band (1.65 $\mu$m) and SOFIA HAWC+ 154 $\mu$m polarization observations of the low-mass core L483. Our H-band observations reveal a magnetic field that is overwhelmingly in the E-W direction, which is approximately parallel to the bipola
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3b5955e12f75d605a0a31c72f5d7dd7f
http://arxiv.org/abs/2206.00683
http://arxiv.org/abs/2206.00683
Autor:
Ian W. Stephens, Philip C. Myers, Catherine Zucker, James M. Jackson, B.-G. Andersson, Rowan Smith, Archana Soam, Cara Battersby, Patricio Sanhueza, Taylor Hogge, Howard A. Smith, Giles Novak, Sarah Sadavoy, Thushara G.S. Pillai, Zhi-Yun Li, Leslie W. Looney, Koji Sugitani, Simon Coudé, Andrés Guzmán, Alyssa Goodman, Takayoshi Kusune, Fábio P. Santos, Leah Zuckerman, Frankie Encalada
Publikováno v:
The Astrophysical Journal Letters. 926:L6
Star formation primarily occurs in filaments where magnetic fields are expected to be dynamically important. The largest and densest filaments trace spiral structure within galaxies. Over a dozen of these dense ($\sim$10$^4$\,cm$^{-3}$) and long ($>$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ebbd8b6a90ec04071579718771a03c5b
https://doi.org/10.3847/2041-8213/ac4d8f
https://doi.org/10.3847/2041-8213/ac4d8f
