Zobrazeno 1 - 10
of 25
pro vyhledávání: '"Josep M. Masqué"'
Autor:
Jazmín Ordóñez-Toro, Sergio A. Dzib, Laurent Loinard, Gisela Ortiz-León, Marina A. Kounkel, Josep M. Masqué, S.-N. X. Medina, Phillip A. B. Galli, Trent J. Dupuy, Luis F. Rodríguez, Luis H. Quiroga-Nuñez
Publikováno v:
The Astronomical Journal, Vol 167, Iss 3, p 108 (2024)
We report dynamical mass measurements of the individual stars in the most luminous and massive stellar member of the nearby Ophiuchus star-forming region, the young tight binary system S1. We combine 28 archival data sets with seven recent proprietar
Externí odkaz:
https://doaj.org/article/f218085a0c914e1fb7f3664b1825da6b
Autor:
Geovanni Cortes-Rangel, Luis A. Zapata, Pedro R. Rivera-Ortiz, Megan Reiter, Satoko Takahashi, Josep M. Masqué
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 2, p 193 (2023)
We present a study of six dusty and gaseous pillars (containing the Herbig–Haro (HH) objects HH 1004 and HH 1010) and globules (that contain the HH 666, HH 900, HH 1006, and HH 1066 objects) localized in the Carina Nebula using sensitive and high-a
Externí odkaz:
https://doaj.org/article/f4a8c0eea53343bc8a049b20163647d8
Autor:
Miguel A. Trinidad, Stanley E. Kurtz, Josep M. Masqué, S. N. X. Medina, Laurent Loinard, Luis F. Rodríguez, Carlos A. Rodríguez-Rico, Sergio A. Dzib
Publikováno v:
Revista Mexicana de Astronomía y Astrofísica. 57:81-89
We present Very Large Array 7 mm continuum observations of four Ultra-Compact (UC)HII regions, observed previously at 1.3 cm, in order to investigate the nature of the compact radio sources associated with these regions. We detected a total of seven
Autor:
Vanessa Yanza, Josep M. Masqué, Sergio A. Dzib, Luis F. Rodríguez, S.-N. X. Medina, Stan Kurtz, Laurent Loinard, Miguel A. Trinidad, Karl M. Menten, Carlos A. Rodríguez-Rico
We present a catalog of radio sources of the M 17 region based on deep X band radio observations centered at 10 GHz obtained with the Jansky Very Large Array in the A configuration. We detect a total of 194 radio sources, 12 of them extended and 182
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f365914e16a9352be12ffcd827c9001
http://arxiv.org/abs/2204.09555
http://arxiv.org/abs/2204.09555
Autor:
M. A. Trinidad, Josep M. Masqué, C. H. Ishwara-Chandra, Tatiana Rodríguez-Esnard, S. Jeyakumar
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 483:1184-1191
We report continuum GMRT observations aimed to explore the behavior of the jet associated with IRAS 16547-4247 at very low frequencies (325 MHz and 610 MHz). The obtained maps reveal an elongated morphology in the SE-NW direction. In addition, the 61
Autor:
Satoko Takahashi, Geovanni Cortes-Rangel, Adal Mesa-Delgado, Jesús A. Toalá, Luis A. Zapata, Josep M. Masqué, Paul T. P. Ho
Publikováno v:
The Astronomical Journal. 159:62
We present Atacama Large Millimeter/Submillimeter Array (ALMA) 1.3 mm continuum and C$^{18}$O(2$-$1), N$_2$D$^{+}$(3$-$2), $^{13}$CS(5$-$4), and $^{12}$CO(2$-$1) line sensitive and high angular resolution ($\sim$0.3$''$) observations of the famous ca
We present sensitive high angular resolution ($\sim$ 0.1$''$ -- 0.3$''$) continuum ALMA (The Atacama Large Millimeter/Submillimeter Array) observations of the archetypal hot core located in Orion-KL. The observations were made in five different spect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c76b90c3fcc9fbf6f930948ba4595527
Publikováno v:
Proceedings of the International Astronomical Union. 13:315-316
We present radio continuum and water maser observations toward the high-mass star-forming region IRAS 23151+5912 from the VLA and VLBA archive, respectively. We detected a continuum source, which seems to be a hypercompact HII region. In addition, a
Autor:
P. Frau, Álvaro Sánchez-Monge, Felipe O. Alves, Oscar Morata, Robert Estalella, Josep M. Girart, Gabriel A. P. Franco, Maria T. Beltrán, Josep M. Masqué, Gemma Busquet
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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The Pipe Nebula is a massive, nearby dark molecular cloud with a low star-formation efficiency which makes it a good laboratory to study the very early stages of the star formation process. The Pipe Nebula is largely filamentary, and appears to be th
Publikováno v:
The Astrophysical Journal. 695:1505-1516
We present a Berkeley-Illinois-Maryland Association (BIMA) Array molecular survey of the star forming core ahead of HH 80N, the optically obscured northern counterpart of the Herbig-Haro objects HH 80/81. Continuum emission at 1.4 mm and 8 micron is