Zobrazeno 1 - 10
of 63
pro vyhledávání: '"Roberto Claudio Gamen"'
Autor:
Silvina Cichowolski, S B Cárdenas, L. Rizzo, J. A. Molina Lera, L. A. Suad, Roberto Claudio Gamen
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 509:3395-3409
We present a multiwavelength investigation of the H ii region G347.600+00.211, located at a distance of 7.9 kpc. We analyse the gas and dust properties aiming to disentangle the origin of the region as well as its role in the formation of new stars.
Autor:
Rodolfo H. Barbá, Philip Massey, Roberto Claudio Gamen, Omar Gustavo Benvenuto, G. Ferrero, Nidia Morrell, C. Rodriguez, José Ignacio Arias
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 508:2179-2193
We present a comprehensive study of the massive binary system HM1~8, based on multi-epoch high resolution spectroscopy, $V$-band photometry and archival X-ray data. Spectra from the OWN Survey, a high resolution optical monitoring of Southern O and W
Autor:
Nolan R. Walborn, Rodolfo H. Barbá, Nidia Morrell, José Ignacio Arias, Roberto Claudio Gamen, Chris Evans, Yaël Nazé, Jan Cami, Gregg A. Wade, Amin Farhang, I. D. Howarth, Jonathan Smoker, Nick L. J. Cox
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 483:2581-2591
We report new spectroscopic observations of the magnetic Of?p star HD 148937 obtained since 2015 that differ qualitatively from its extensive historical record of weak, periodic spectral variations. This remarkable behaviour represents clear evidence
Autor:
C. Sabin-Sanjulian, M. V. McSwain, C. Putkuri, Nidia Morrell, Rodolfo H. Barbá, Alexander W. Fullerton, S. S. Diaz, G. Ferrero, Tabetha S. Boyajian, J. Maíz Apellániz, José Ignacio Arias, Roberto Claudio Gamen
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
Digital.CSIC. Repositorio Institucional del CSIC
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
Digital.CSIC. Repositorio Institucional del CSIC
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
HD 54662 AB is one of the three O + OB binaries known so far with orbital period longer than 1000 d, offering the opportunity to test scenarios of massive star formation and models of single stellar evolution. Here, we present a detailed study of thi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d10fc6b31968aab6648543d94cbda29
https://academic.oup.com/mnras/article/494/3/3937/5825374
https://academic.oup.com/mnras/article/494/3/3937/5825374
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 480:2386-2404
Fil: Molina Lera, Jose Alejo. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico Conicet - La Plata. Instituto de Astrofisica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronomicas y Geofi
Autor:
Rodolfo H. Barbá, C. Putkuri, Roberto Claudio Gamen, Nidia Morrell, Omar Gustavo Benvenuto, José Ignacio Arias
Publikováno v:
Astronomy & Astrophysics. 650:A96
Context. The OWN Survey has detected several O-type stars with composite spectra whose individual components show very different line broadening. Some of these stars have been revealed as binary systems whose components are asynchronous. This fact ma
In the pre-main-sequence stage, star-disc interactions have been shown to remove stellar angular momentum and regulate the rotation periods of stars with M2 and earlier spectral types. Whether disc regulation also extends to stars with later spectral
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::845f893da4b9e8cd89bfe22d3d5f7856
http://arxiv.org/abs/1905.10312
http://arxiv.org/abs/1905.10312
Autor:
J. Lorenzo, Amparo Marco, E. Trigueros Páez, C. Fariña, Sergio Simón-Díaz, J. Salas, A. Herrero, Julia Ines Arias, Ignacio Negueruela, Alfredo Sota, Roberto Claudio Gamen, Jose A. Caballero, Nidia Morrell, Rodolfo H. Barbá, J. Maíz Apellániz, Emilio J. Alfaro, Anne Pellerin
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universidad de Alicante (UA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
RUA. Repositorio Institucional de la Universidad de Alicante
Instituto Nacional de Técnica Aeroespacial (INTA)
Universidad de Alicante (UA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
RUA. Repositorio Institucional de la Universidad de Alicante
Instituto Nacional de Técnica Aeroespacial (INTA)
This article has an erratum: A&A 639: C1 (2020)
Context. Multiplicity in massive stars is key to understanding the chemical and dynamical evolution of galaxies. Among massive stars, those of O type play a crucial role due to their high masses an
Context. Multiplicity in massive stars is key to understanding the chemical and dynamical evolution of galaxies. Among massive stars, those of O type play a crucial role due to their high masses an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3dacfaab47c98e1feb433c6f68b0186
http://arxiv.org/abs/1904.11385
http://arxiv.org/abs/1904.11385
Autor:
Roberto Claudio Gamen, Gloria Koenigsberger, Rodolfo H. Barbá, Yaël Nazé, D. J. Hillier, Nidia Morrell
Publikováno v:
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Universidad Nacional de La Plata
instacron:UNLP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The Small Magellanic Cloud multiple system HD 5980 contains a luminous blue variable (LBV) that underwent a major eruption in 1994, and whose current spectrum is that of a hydrogen-rich Wolf–Rayet (WR) star. Since the eruption, the wind mass-loss r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::395b113031bef98b6eed8617481c3f33
http://sedici.unlp.edu.ar/handle/10915/123486
http://sedici.unlp.edu.ar/handle/10915/123486