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(created 2025-01-27T14:00:25Z)
https://docs.google.com/spreadsheets/d/1Wm-7hEf2TLorQgigqE8ncOh1h8hLxxBBmaXXM7tmA8w/edit?usp=sharing
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Justin A. Kader, Vivian U, Jeffrey A. Rich, Marina Bianchin, Sean T. Linden, Anne M. Medling, Tanio Diaz-Santos, George C. Privon et al.
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Jonah C. Rose, Mariangela Lisanti, Paul Torrey, Francisco Villaescusa-Navarro, Alex M. Garcia, Arya Farahi, Carrie Filion, Alyson M. Brooks et al.
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Alex M. Garcia, Paul Torrey, Aniket Bhagwat, Xuejian Shen, Mark Vogelsberger, William McClymont, Jaya Nagarajan-Swenson, Sophia G. Ridolfo et al.
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Desika Narayanan, Paul Torrey, Daniel Stark, John Chisholm, Steven Finkelstein, Alex Garcia, Jessica Kelley-Derzon, Federico Marinacci et al.
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Luke Xia, M. Swisdak
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Yi-Ying Wang, Lei Lei, Shao-Peng Tang, Yi-Zhong Fan
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Ming-Xuan Lu, Yun-Feng Liang, Xiang-Gao Wang, Hao-Qiang Zhang
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Author:
Prasad Mani, Timothy R. Bedding, Mara Bernizzoni, Simon J. Murphy, Daniel Hey
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Jinghao Zhang, Yacheng Kang, Jiahang Zhong, Hong-Bo Li, Liang-Duan Liu, Yun-Wei Yu, Lijing Shao
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4 years ago
Title: History of the solar nebula from meteorite paleomagnetism Benjamin P. Weiss+
Link: https://advances.sciencemag.org/content/7/1/eaba5967
Description: We review recent advances in our understanding of magnetism in the solar nebula and protoplanetary disks (PPDs). We discuss the implications of theory, meteorite measurements, and astronomical observations for planetary formation and nebular evolution. Paleomagnetic measurements indicate the presence of fields of 0.54 ± 0.21 G at ~1 to 3 astronomical units (AU) from the Sun and ≳0.06 G at 3 to 7 AU until >1.22 and >2.51 million years (Ma) after solar system formation, respectively. These intensities are consistent with those predicted to enable typical astronomically observed protostellar accretion rates of ~10−8 M⊙year−1, suggesting that magnetism played a central role in mass transport in PPDs. Paleomagnetic studies also indicate fields <0.006 G and <0.003 G in the inner and outer solar system by 3.94 and 4.89 Ma, respectively, consistent with the nebular gas having dispersed by this time. This is similar to the observed lifetimes of extrasolar protoplanetary disks.
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Votes: 1
4 years ago Author:
Ava Nederlander, A. Meredith Hughes, Anna J. Fehr, Kevin M. Flaherty, Kate Y. L. Su, Attila Moor, Eugene Chiang, Sean M. Andrews et al.
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Votes: 2
4 years ago Author:
Tim Lichtenberg, Joanna Drazkowska, Maria Schönbächler, Gregor J. Golabek, Thomas O. Hands
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Votes: 1
4 years ago
Title:
A Smoking Gun for Planetesimal Formation: Charge Driven Growth into a
New Size Range
(View PDF)
Author:
Jens Teiser, Maximilian Kruss, Felix Jungmann, Gerhard Wurm
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Votes: 1
4 years ago Author:
Md Abul Hayat, George Stein, Peter Harrington, Zarija Lukić, Mustafa Mustafa
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Votes: 1
4 years ago
Title:
Sub-arcsecond Imaging of the Complex Organic Chemistry in Massive
Star-forming Region G10.6-0.4
(View PDF)
Author:
Charles J. Law, Qizhou Zhang, Karin I. Öberg, Roberto Galván-Madrid, Eric Keto, Hauyu Baobab Liu, Paul T. P. Ho
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Votes: 2
4 years ago
Title:
FAUST II. Discovery of a Secondary Outflow in IRAS 15398-3359:
Variability in Outflow Direction during the Earliest Stage of Star Formation?
(View PDF)
Author:
Yuki Okoda, Yoko Oya, Logan Francis, Doug Johnstone, Shu-ichiro Inutsuka, Cecilia Ceccarelli, Claudio Codella, Claire Chandler et al.
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Votes: 2
4 years ago
Title:
Evolutionary Map of the Universe (EMU):Compact radio sources in the
SCORPIO field towards the Galactic plane
(View PDF)
Author:
S. Riggi, G. Umana, C. Trigilio, F. Cavallaro, A. Ingallinera, P. Leto, F. Bufano, R. P. Norris et al.
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Votes: 1
4 years ago
Title:
Low star formation efficiency due to turbulent adiabatic compression in
the Taffy bridge
(View PDF)
Author:
B. Vollmer, J. Braine, B. Mazzilli-Ciraulo, B. Schneider
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Votes: 1
4 years ago Author:
Jamila Pegues, Ian Czekala, Sean M. Andrews, Karin I. Öberg, Gregory J. Herczeg, Jennifer B. Bergner, L. Ilsedore Cleeves, Viviana V. Guzmán et al.
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