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pro vyhledávání: '"R Leo"'
Mapping magnetic fields is the key to resolving what remains an unclear physical picture of circumstellar magnetic fields in late-type evolved stars. Observations of linearly polarized emission from thermal molecular line transitions due to the Goldr
Externí odkaz:
http://arxiv.org/abs/2007.00215
Autor:
Fonfría, J. P., Santander-García, M., Cernicharo, J., Velilla-Prieto, L., Agúndez, M., Marcelino, N., Quintana-Lacaci, G.
Publikováno v:
A&A 622, L14 (2019)
We present new interferometer molecular observations of R Leo taken at 1.2 mm with the Atacama Large Millimeter Array with an angular resolution up to ~0.026 arcsec. These observations permit us to resolve the innermost envelope of this star revealin
Externí odkaz:
http://arxiv.org/abs/1902.02574
The origin of magnetism around AGB stars is uncertain. If these stars drive a dynamo, it cannot be sufficient to generate a strong global field, otherwise the observed X-ray luminosities would be higher. Other explanations for the circular polarizati
Externí odkaz:
http://arxiv.org/abs/0809.0359
The study of the innermost circumstellar layers around AGB stars is crucial to understand how these envelopes are formed and evolve. The SiO maser emission occurs at a few stellar radii from the central star, providing direct information on the stell
Externí odkaz:
http://arxiv.org/abs/0704.0682
Autor:
Carli M. Stewart, Elizabeth L. Siegler, R. Leo Sakemura, Michelle J. Cox, Truc Huynh, Brooke Kimball, Long Mai, Ismail Can, Claudia Manriquez Roman, Kun Yun, Olivia Sirpilla, James H. Girsch, Ekene Ogbodo, Wazim Mohammed Ismail, Alexandre Gaspar-Maia, Justin Budka, Jenny Kim, Nathalie Scholler, Mike Mattie, Simone Filosto, Saad S. Kenderian
Publikováno v:
Nature Communications, Vol 15, Iss 1, Pp 1-17 (2024)
Abstract Durable response to chimeric antigen receptor T (CART) cell therapy remains limited in part due to CART cell exhaustion. Here, we investigate the regulation of CART cell exhaustion with three independent approaches including: a genome-wide C
Externí odkaz:
https://doaj.org/article/9385e305f428439ba7536b1503dee2fa
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
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Mapping magnetic fields is the key to resolving the unclear physical picture of circumstellar magnetic fields in late-type evolved stars. Observations of linearly polarized emission from thermal molecular line transitions due to the Goldreich-Kylafis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35b9bf1a348e7f94144cdfafc23aea0e
http://arxiv.org/abs/2007.00215
http://arxiv.org/abs/2007.00215
Mapping magnetic fields is the key to resolving what remains an unclear physical picture of circumstellar magnetic fields in late-type evolved stars. Observations of linearly polarized emission from thermal molecular line transitions due to the Goldr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6c76a3f0fb043255b7a5646517405414
Akademický článek
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Autor:
Fonfría, José Pablo, Santander-García, M., Cernicharo, José, Velilla Prieto, L., Agúndez, Marcelino, Quintana-Lacaci, G.
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
ALMA 2019, Cagliari, Italy 14–18 October 2019
Asymptotic Giant Branch stars (AGBs) display roughly spherically symmetric circumstellar envelopes (CSEs) composed of expanding molecular gas and dust. Nevertheless, several AGB stars have been fou
Asymptotic Giant Branch stars (AGBs) display roughly spherically symmetric circumstellar envelopes (CSEs) composed of expanding molecular gas and dust. Nevertheless, several AGB stars have been fou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e9cc5fe8b93cf41d395d0d972afae11
http://hdl.handle.net/10261/213074
http://hdl.handle.net/10261/213074