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M. Rubio  - - - 
Top co-authors See all
Y. Fukui

318 shared publications

Department of Physics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8601, Japan

Elias Brinks

152 shared publications

University of Hertfordshire, Hatfield, UK

R. H. Barbá

132 shared publications

Departamento de Física y Astronomía, Universidad de la Serena, Av. Juan Cisternas 1200 Norte, La Serena, Chile

Nolan R. Walborn

129 shared publications

Space Telescope Science Institute

Norikazu Mizuno

77 shared publications

National Astronomical Observatory of Japan (NAOJ), National Institutes of Natural Sciences (NINS), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

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Publication Record
Distribution of Articles published per year 
(1998 - 2018)
Total number of journals
published in
 
5
 
Publications See all
Article 0 Reads 0 Citations Massive young stellar objects in the N 66/NGC 346 region of the SMC M. Rubio, R. H. Barbá, V. M. Kalari Published: 01 July 2018
Astronomy and Astrophysics, doi: 10.1051/0004-6361/201730487
DOI See at publisher website
Article 0 Reads 0 Citations Dense Cloud Cores revealed by ALMA CO observations in the low metallicity dwarf galaxy WLM M. Rubio, B. Elmegreen, D. Hunter, J. Cortes, E. Brinks, P. ... Published: 21 March 2016
Proceedings of the International Astronomical Union, doi: 10.1017/S1743921316011650
DOI See at publisher website
BOOK-CHAPTER 0 Reads 0 Citations The Small Magellanic Cloud: Molecular Gas and Star Formation Mónica Rubio Published: 14 November 2014
Lessons from the Local Group, doi: 10.1007/978-3-319-10614-4_25
DOI See at publisher website
Article 0 Reads 1 Citation Discovery of a dense molecular cloud towards a young massive embedded star in 30 Doradus M. Rubio, S. Paron, G. Dubner Published: 22 July 2009
Astronomy and Astrophysics, doi: 10.1051/0004-6361/200810431
DOI See at publisher website ABS Show/hide abstract
Context. The 30 Doradus region in the Large Magellanic Cloud is one of the most outstanding star-forming regions of the Local Group and a primary target for studying star formation in an environment of low metallicity. Aims. To obtain a more complete picture of the cool gas that has not yet been consumed or dispersed, we searched for line emission from molecular clouds that could be associated with molecular hydrogen emission detected in the region. Methods. We obtained a high sensitivity 12CO –1 map with the 15-m SEST telescope, complemented by pointed observations of 13CO –1 and CS –1. Results. We report the discovery of a dense molecular cloud towards an embedded young massive star at ~20” (~5 pc, at the distance of 50 kpc) northwest of R136, the compact massive central stellar cluster powering 30 Doradus in the LMC, which could be triggering star formation in the surrounding molecular clouds. We derived a molecular mass of ≲104 , a linear radius of 3 pc, as an upper limit, and a mean density of ≳103 cm-3 for the cloud. The detection of the CS –1 emission line indicates higher densities, ~106 cm-3. The dense molecular cloud is associated with molecular 2.12 μm H2 emission. We suggest that the observed molecular gas could be the remains of dense molecular material surviving the action of strong UV fields and winds in which the young massive star has formed.
Article 0 Reads 8 Citations Millimeter dust emission from an SMC cold molecular cloud M. Rubio, F. Boulanger, F. Rantakyro, A. Contursi Published: 10 September 2004
Astronomy and Astrophysics, doi: 10.1051/0004-6361:200400046
DOI See at publisher website
Article 0 Reads 3 Citations Near-infrared surface photometry of early-type galaxies J. R. Ducati, S. B. Rembold, M. G. Pastoriza, M. Rubio, M. R... Published: 02 August 2002
Astronomy and Astrophysics, doi: 10.1051/0004-6361:20020904
DOI See at publisher website
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