Zobrazeno 1 - 10
of 127
pro vyhledávání: '"Susana, Lizano"'
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 1, p 32 (2023)
Pseudodisks are dense structures formed perpendicular to the direction of the magnetic field during the gravitational collapse of a molecular cloud core. Numerical simulations of the formation of pseudodisks are usually computationally expensive with
Externí odkaz:
https://doaj.org/article/6928911ac2cd476baaaafd541361e048
It has been proposed that some hot molecular cores (HMCs) harbor a young embedded massive star, which heats an infalling envelope and accretes mass at a rate high enough to ``choke off'' an incipient HII region. This class of HMCs would mark the youn
Externí odkaz:
http://arxiv.org/abs/astro-ph/9909473
Autor:
Adriana R. Rodríguez-Kamenetzky, Carlos Carrasco-González, Luis F. Rodríguez, Tom P. Ray, Alberto Sanna, Luca Moscadelli, Melvin Hoare, Roberto Galván-Madrid, Hsien Shang, Susana Lizano, Jochen Eislöffel, Jeremy Lim, José M. Torrelles, Paul Ho, Anton Feeney-Johansson
We report new VLA and e-MERLIN high-resolution and -sensitivity images of the triple radio continuum source in the Serpens star-forming region. These observations allowed us to perform a deep multifrequency, multiepoch study by exploring the innermos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bdb34116542e6ecb25e35b096d8cc9d0
http://hdl.handle.net/10261/295675
http://hdl.handle.net/10261/295675
Autor:
Susana Lizano, M. Boer, Michael G. Richer, William H. Lee, Alexander Kutyrev, Rosa L. Becerra, Ricardo F. González, D. Turpin, Carlos Román-Zúñiga, Jonathan Granot, Jean-Luc Atteia, Joshua S. Bloom, Jason X. Prochaska, Anabella T. Araudo, Alan M. Watson, Nat Butler, E. Troja, F. De Colle, J. Jesús González, Enrico Ramirez-Ruiz, Nissim Fraija, Alain Klotz, Jorge Cantó
Publikováno v:
Astrophys.J.
Astrophys.J., 2021, 908 (1), pp.39. ⟨10.3847/1538-4357/abcd3a⟩
Astrophys.J., 2021, 908 (1), pp.39. ⟨10.3847/1538-4357/abcd3a⟩
The transition from prompt to the afterglow emission is one of the most exciting and least understood phases in gamma-ray bursts (GRBs). Correlations among optical, X-ray and gamma-ray emission in GRBs have been explored, to attempt to answer whether
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f6e19bc101480fa9e5515041de60cfa
http://arxiv.org/abs/2009.13614
http://arxiv.org/abs/2009.13614
Autor:
Christopher J. Miller, Ezequiel Manzo-Martínez, Nuria Calvet, Paola D'Alessio, Susana Lizano, Cesar Briceno, Jesús Hernández, Ramiro Franco Hernández, Karina Maucó
We present a study of the evolution of the inner few astronomical units of protoplanetary disks around low-mass stars. We consider nearby stellar groups with ages spanning from 1 to 11 Myr, distributed into four age bins. Combining PANSTARSS photomet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::937a6dc259e9a125d8dcf5ffb57fab89
http://arxiv.org/abs/2004.02916
http://arxiv.org/abs/2004.02916
Autor:
Anibal Sierra, Susana Lizano
It is known that the millimeter dust thermal emission of protoplanetary disks is affected by scattering, such that for optically thick disks the emission decreases with respect to the pure absorption case and the spectral indices can reach values bel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9edee6035d1c2bfc45496c136340374d
http://arxiv.org/abs/2003.02982
http://arxiv.org/abs/2003.02982
We present 29SiO(J = 8–7) ν = 0, SiS (J = 19–18) ν = 0, and 28SiO (J = 8–7) ν = 1 molecular line archive observations made with the Atacama Large Millimeter/Submillimeter Array (ALMA) of the molecular outflow associated with Orion Source I.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68a64e84062934d4b769b9b5c88bac15
Autor:
Susana Lizano, Luis F. Rodríguez, J. C. Rodríguez-Ramírez, Jorge Cantó, Alejandro C. Raga, A. Tinoco-Arenas
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 471:4910-4916
We model the ALMA and VLA millimeter radial profiles of the disk around HL Tau to constrain the properties of the dust grains. We adopt the disk evolutionary models of Lynden-Bell \& Pringle and calculate their temperature and density structure and e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b4312ff4c740fac759c11742f44d8af
Autor:
Estela Susana Lizano Soberón
En su discurso de ingreso, la doctora Estela Susana Lizano Soberón expone brevemente su trayectoria académica, así como los retos que tuvo que enfrentar durante su formación por el desarrollo incipiente que tenía en ese momento la astronomía en