Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Gabriel A. P. Franco"'
Autor:
Lílian da Cruz Assis, Breno Willian França Silveira, Heloá de Amorim Peres Lima, Lorena Daiza Aquino Ferraz, Lucas Gabriel de Melo Franco
Publikováno v:
Bionorte, Vol 9, Iss S2 (2022)
Objetivo: relatar o processo de criação de uma liga acadêmica em período pandêmico. Materiais e Métodos: trata-se de um relato de experiência da criação da Liga Acadêmica de Prótese e Reabilitação Oral (LAPRO/FUNORTE) no período de 4 de
Externí odkaz:
https://doaj.org/article/b9c8f85913d24448b825bfdf53a6344c
Autor:
Koji Sugitani, Stefan Reissl, Jonathan D. Henshaw, Dan P. Clemens, Karl M. Menten, Fumitaka Nakamura, Enrique Lopez-Rodriguez, Jens Kauffmann, Helmut Wiesemeyer, Felipe O. Alves, Daniel Seifried, Gabriel A. P. Franco, Philip C. Myers, Thushara Pillai
Publikováno v:
Nature Astronomy. 4:1195-1201
Observations indicate that molecular clouds are strongly magnetized, and that magnetic fields influence the formation of stars. A key observation supporting the conclusion that molecular clouds are significantly magnetized is that the orientation of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d1476e1f1e8f381b36ebf99a73e5d7a
https://doi.org/10.1038/s41550-020-1172-6
https://doi.org/10.1038/s41550-020-1172-6
Autor:
Antonio Garufi, Zhaohuan Zhu, Alice Zurlo, Gabriel A. P. Franco, Josep M. Girart, Sebastian Perez, Felipe O. Alves, L. Ilsedore Cleeves
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The presence of planets or substellar objects still embedded in their native protoplanetary disks is indirectly suggested by disk substructures like gaps, cavities, and spirals. However, these companions are rarely detected. We present Very Large Tel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d5c37e4ad7c4e4352fa1b543e424dad
http://arxiv.org/abs/2103.03881
http://arxiv.org/abs/2103.03881
Autor:
Zhaohuan Zhu, Alice Zurlo, L. Ilsedore Cleeves, Josep M. Girart, Felipe O. Alves, Gabriel A. P. Franco, Paola Caselli
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
The Astrophysical Journal Letters
The Astrophysical Journal Letters, 2020, 904, ⟨10.3847/2041-8213/abc550⟩
instname
The Astrophysical Journal Letters
The Astrophysical Journal Letters, 2020, 904, ⟨10.3847/2041-8213/abc550⟩
While it is widely accepted that planets are formed in protoplanetary disks, there is still much debate on when this process happens. In a few cases protoplanets have been directly imaged, but for the vast majority of systems, disk gaps and cavities
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::812056028dcbd9e9e17e6e0c7a99f5ac
http://hdl.handle.net/10261/236116
http://hdl.handle.net/10261/236116
Autor:
Bo Zhao, Josep M. Girart, Anika Schmiedeke, Dominique Segura-Cox, Felipe O. Alves, Gabriel A. P. Franco, Paola Caselli
Publikováno v:
Science (New York, N.Y.). 366(6461)
The majority of stars are part of gravitationally bound stellar systems, such as binaries. Observations of protobinary systems constrain the conditions that lead to stellar multiplicity and subsequent orbital evolution. We report high-angular resolut
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ac35712d5651f09ace19c5810d6fb9f3
https://pubmed.ncbi.nlm.nih.gov/31604307
https://pubmed.ncbi.nlm.nih.gov/31604307
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 462:2266-2274
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d87553531f9cc8f886c594785dcc2013
https://doi.org/10.1093/mnras/stw1666
https://doi.org/10.1093/mnras/stw1666
Autor:
Marco Padovani, Felipe O. Alves, Wouter Vlemmings, Gabriel A. P. Franco, P. Caselli, Daniele Galli, Qizhou Zhang, Helmut Wiesemeyer, Josep M. Girart
Publikováno v:
Astronomy & Astrophysics
We use polarization observations of a circumbinary disk to investigate how the polarization properties change at distinct frequency bands. Our goal is to discern the main mechanism responsible for the polarization through comparison between our obser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b485c4e7d9ad1c416f3b38bafea123b0
http://arxiv.org/abs/1805.00494
http://arxiv.org/abs/1805.00494
Autor:
J. F. C. Santos, F. F. S. Maia, Alexandre Roman-Lopes, J. Vargas-González, Fabio P. Santos, Gabriel A. P. Franco, David Sanmartim
We carried out an optical polarimetric study in the direction of the RCW95 star forming region in order to probe the sky-projected magnetic field structure by using the distribution of linear polarization segments which seem to be well aligned with t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6eec00c78b9c4d6e535e998d6b2411ad
Autor:
Marc-Antoine Miville-Deschênes, Patrick Hennebelle, Peter G. Martin, Vincent Guillet, E. Falgarone, F. Boulanger, Juan D. Soler, Felipe O. Alves, Gabriel A. P. Franco, Andrea Bracco, François Levrier
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2016, 596, pp.A93. ⟨10.1051/0004-6361/201628996⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 596, pp.A93. ⟨10.1051/0004-6361/201628996⟩
Astronomy and Astrophysics-A&A, 2016, 596, pp.A93. ⟨10.1051/0004-6361/201628996⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 596, pp.A93. ⟨10.1051/0004-6361/201628996⟩
Within four nearby (d < 160 pc) molecular clouds, we statistically evaluate the structure of the interstellar magnetic field, projected on the plane of the sky and integrated along the line of sight, as inferred from the polarized thermal emission of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7c5eee2010ac4060dc8655f3ef60c26
https://hal.sorbonne-universite.fr/hal-01465843
https://hal.sorbonne-universite.fr/hal-01465843
Publikováno v:
NASA Astrophysics Data System
The G14.225-0.506 infrared dark cloud (IRDC G14.2) displays a remarkable complex of parallel dense molecular filaments projected on the plane of the sky. Previous dust emission and molecular-line studies have speculated whether magnetic fields could
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d1da5328a0daf4a63ba01162c6d3acb