Browsing by Author "Rubio López, Mónica"

Now showing items 1-20 of 36

    • A study of the invisible circum-galactic medium around A z=0.77 star-forming galaxy using gravitational-ARC ... 
      Fernández Figueroa, Antonia Isabel (Universidad de Chile, 2021)
      Gravitational arc-tomography is a novel technique that allows one to study the absorbing high-redshift circum-galactic medium (CGM) in a two-dimensional fashion by using giant gravitational arcs as background sources. ...
    • A (C-12)O survey of the Small Magellanic Cloud 
      Rubio López, Mónica; Garay Brignardello, Guido; Montani, J.; Thaddeus, P. (1991-02-10)
      The central 2 arcsec x 2 arcsec region of the SMC has been fully surveyed to search for (C-12)O emission in the J = 1-0 transition. (C-12)O emission from two large complexes located in the southwest and northeast regions ...
    • Carbon monoxide in clouds at low metallicity in the dwarf irregular galaxy WLM 
      Elmegreen, Bruce; Rubio López, Mónica; Hunter, Deidre; Verdugo, Celia; Brinks, Elias; Schruba, Andreas (Nature, 2013)
      Carbon monoxide (CO) is the primary tracer for interstellar clouds where stars form, but it has never been detected in galaxies in which the oxygen abundance relative to hydrogen is less than 20 per cent of that of the ...
    • Characterizing substructures and interactions in the disks around multiple stellar systems 
      Troncoso Kurtovic, Nicolás Gustavo (Universidad de Chile, 2019)
      Para caracterizar las subestructuras inducidas en discos protoplanetarios por la interacción entre estrellas en sistemas multiples, estudiamos la emisión de continuo en $1.25\,$mm y la linea de emisión molecular $^{12}$CO(J:2-1) ...
    • CHARACTERIZING THE LOW-MASS MOLECULAR COMPONENT IN THE NORTHERN SMALL MAGELLANIC CLOUD 
      Muller, E.; Ott, Jürgen; Hughes, A.; Pineda, J. L.; Wong, T.; Mizuno, Norikazu; Kawamura, Akiko; Mizuno, Y.; Fukui, Yasuo; Onishi, T.; Rubio López, Mónica (2010-01-26)
      We present here the first results from a high-resolution survey of the 12CO(J=1-0) emission across the northern part of the poorly-enriched Small Magellanic Cloud, made with the ATNF Mopra telescope. Three molecular ...
    • CO and CS in the Magellanic Clouds: ax(2)-analysis of multitransitional data based on the MEP radiative ... 
      Nikolic, Silvana; Garay Brignardello, Guido; Rubio López, Mónica; Johansson, L. E. B. (2007)
      Aims. Our goal is to determine the physical properties of molecular gas located in different environments of the SMC-from near the vicinity of hot HII regions to cold, quiescent clouds - via modelling and simulations, and ...
    • (CO)-C-12(3-2) emission in spiral galaxies: Warm molecular gas in action? 
      Galaz, Gaspar, 1967-; Cortés, Paulo; Bronfman Aguiló, Leonardo; Rubio López, Mónica (UNIV CHICAGO PRESS, 2008-04-10)
      Using the APEX submillimeter telescope we have investigated the (CO)-C-12(3-2) emission in five face-on nearby barred spiral galaxies, where three of them are high surface brightness galaxies (HSBs) lying at the Freeman ...
    • Cold dust clumps in dynamically hot gas 
      Kim, S.; Kwon, E.; Madden, S. C.; Meixner, M.; Hony, S.; Panuzzo, P.; Sauvage, M.; Roman Duval, Julia; Gordon, K. D.; Engelbracht, C.; Israel, F. P.; Misselt, K.; Okumura, K.; Li, A.; Bolatto, Alberto; Skibba, R.; Galliano, F.; Matsuura, M.; Bernard, J. P.; Bot, Caroline; Galametz, M.; Hughes, A.; Kawamura, A.; Onishi, T.; Paradis, D.; Poglitsch, A.; Reach, W. T.; Robitaille, T.; Rubio López, Mónica; Tielens, A. G. G. M. (EDP Sciences, 2010-07)
      Aims. We present clumps of dust emission from Herschel observations of the Large Magellanic Cloud (LMC) and their physical and statistical properties. We catalog cloud features seen in the dust emission from Herschel ...
    • A complete CO survey of the Large Magellanic Cloud 
      Cohen, R. S.; Dame, T. M.; Garay Brignardello, Guido; Montani, J.; Rubio López, Mónica; Thaddeus, P. (1988-08-15)
      A complete CO survey of the central 6 deg x 6 deg of the LMC was performed in order to determine the distribution of molecular clouds. At least 10 percent of the region studied exhibits CO line emission, with peak line ...
    • DENSE CLUMPS IN GIANT MOLECULAR CLOUDS IN THE LARGE MAGELLANIC CLOUD: DENSITY AND TEMPERATURE DERIVED FROM ... 
      Minamidani, Tetsuhiro; Tanaka, Takanori; Mizuno, Yoji; Mizuno, Norikazu; Kawamura, Akiko; Onishi, Toshikazu; Hasegawa, Tetsuo; Tatematsu, Ken’ichi; Takekoshi, Tatsuya; Sorai, Kazuo; Moribe, Nayuta; Torii, Kazufumi; Sakai, Takeshi; Muraoka, Kazuyuki; Tanaka, Kunihiko; Ezawa, Hajime; Kohno, Kotaro; Kim, Sungeun; Rubio López, Mónica; Fukui, Yasuo (IOP PUBLISHING LTD, 2011-03)
      In order to precisely determine the temperature and density of molecular gas in the Large Magellanic Cloud, we made observations of the optically thin (13)CO(J = 3-2) transition using the ASTE 10 m telescope toward nine ...
    • Determining dust temperatures and masses in the Herschel era: The importance of observations longward of 200 micron 
      Gordon, K. D.; Galliano, F.; Hony, S.; Bernard, J. P.; Bolatto, Alberto; Bot, Caroline; Engelbracht, C.; Hughes, A.; Israel, F. P.; Kemper, F.; Kim, S.; Li, A.; Madden, S. C.; Matsuura, M.; Meixner, M.; Misselt, K.; Okumura, K.; Panuzzo, P.; Rubio López, Mónica; Reach, W. T.; Roman Duval, Julia; Sauvage, M.; Skibba, R.; Tielens, A. G. G. M. (ESO, 2010)
      The properties of the dust grains (e.g., temperature and mass) can be derived from fitting far-IR SEDs (≥100 μm). Only with SPIRE on Herschel has it been possible to get high spatial resolution at 200 to 500 μm that is ...
    • Erratum: “The Herschel inventory of the agents of galaxy evolution (Heritage) in The Magellanic Clouds, a ... 
      Meixner, M.; Panuzzo, P.; Roman Duval, Julia; Engelbracht, C.; Babler, B.; Seale, J.; Hony, S.; Montiel, E.; Sauvage, M.; Gordon, K.; Misselt, K.; Okumura, K.; Chanial, P.; Beck, T.; Bernard, J.; Bolatto, A.; Bot, C.; Boyer, M.; Carlson, L.; Clayton, G.; Chen, C.; Cormier, D.; Fukui, Y.; Galametz, M.; Galliano, F.; Hora, J.; Hughes, A.; Indebetouw, R.; Israel, F.; Kawamura, A.; Kemper, F.; Kim, S.; Kwon, E.; Lebouteiller, V.; Li, A.; Long, K.; Madden, S.; Matsuura, M.; Muller, E.; Oliveira, J.; Onishi, T.; Otsuka, M.; Paradis, D.; Poglitsch, A.; Reach, W.; Robitaille, T.; Rubio López, Mónica; Sargent, B.; Sewilo, M.; Skibba, R.; Smith, L.; Srinivasan, S.; Tielens, A.; van Loon, J.; Whitney, B. (IOP PUBLISHING, 2015)
    • HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE): The Large Magellanic Cloud dust 
      Meixner, M.; Galliano, F.; Hony, S.; Roman Duval, Julia; Robitaille, T.; Panuzzo, P.; Sauvage, M.; Gordon, K.; Engelbracht, C.; Misselt, K.; Okumura, K.; Beck, T.; Bernard, J. P.; Bolatto, Alberto; Bot, Caroline; Boyer, M.; Bracker, S.; Carlson, L. R.; Clayton, G. C.; Chen, C.-H. R.; Churchwell, E.; Fukui, Y.; Galametz, M.; Hora, J. L.; Hughes, A.; Indebetouw, R.; Israel, F. P.; Kawamura, A.; Kemper, F.; Kim, S.; Kwon, E.; Lawton, B.; Li, A.; Long, K. S.; Marengo, M.; Madden, S. C.; Matsuura, M.; Oliveira, J. M.; Onishi, T.; Otsuka, M.; Paradis, D.; Poglitsch, A.; Riebel, D.; Reach, W. T.; Rubio López, Mónica; Sargent, B.; Sewiło, M.; Simon, J. D.; Skibba, R.; Smith, L. J.; Srinivasan, S.; Tielens, A. G. G. M.; van Loon, J. Th.; Whitney, B.; Woods, P. M. (EDP SCIENCES S A., 2010-07)
      The HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE) of the Magellanic Clouds will use dust emission to investigate the life cycle of matter in both the Large and Small Magellanic Clouds (LMC and SMC). Using ...
    • THE HERschel inventory of the agents of galaxy evolution in the magellanic clouds, a herschel open time key program 
      Meixner, M.; Panuzzo, P.; Roman Duval, Julia; Engelbracht, C.; Babler, B.; Seale, J. P.; Hony, S.; Montiel, E.; Sauvage, M.; Gordon, K.; Misselt, K.; Okumura, K.; Chanial, P.; Beck, T.; Bernard, J. P.; Bolatto, A.; Bot, C.; Boyer, M. L.; Carlson, L. R.; Clayton, G. C.; Chen, C.-H. R.; Cormier, D.; Fukui, Y.; Galametz, M.; Galliano, F.; Hora, J. L.; Hughes, A.; Indebetouw, R.; Israel, F.P.; Kawamura, A.; Kemper, F.; Kim, S.; Kwon, E.; Lebouteiller, V.; Li, A.; Long, K. S.; Madden, S. C.; Matsuura, M.; Muller, E.; Oliveira, J. M.; Onishi, T.; Otsuka, M.; Paradis, D.; Poglitsch, A.; Reach, W. T.; Robitaille, T. P.; Rubio López, Mónica; Sargent, B.; Sewiłlo, M.; Skibba, R.; Smith, L.; Srinivasan, S.; Tielens, A.; van Loon, J. Th.; Whitney, B. (The American Astronomical Society, 2013)
      We present an overview of the HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE) in the Magellanic Clouds project, which is a Herschel Space Observatory open time key program. We mapped the Large Magellanic ...
    • High resolution CO observations towards the Bright Eastern Knot of the SNR Puppis A 
      Paron, S.; Dubner, G.; Reynoso, E.; Rubio López, Mónica (EDP SCIENCES S A, 2008-03)
      Aims. This paper reports molecular observations towards the Bright Eastern Knot (BEK) in the SNR Puppis A, a feature where radio and X-ray studies suggest that the shock front is interacting with a dense molecular ...
    • The infrared Hourglass cluster in M8 
      Arias, José I.; Barbá, R. H.; Maíz Apellániz, J.; Morrell, Nidia; Rubio López, Mónica (BLACKWELL PUBLISHING, 2006-03-01)
      A detailed study of the Hourglass nebula in the M8 star-forming region is presented. The study is mainly based on recent subarcsec-resolution JHK(s) images taken at Las Campanas Observatory and complemented with archival ...
    • ISOCAM mid-infrared spectroscopy and NIR photometry of the HII complex N4 in the Large Magellanic Cloud 
      Contursi, A.; Rubio López, Mónica; Sauvage, M.; Cesarsky, D.; Barbá, R. H.; Boulanger, Francois (2007)
      Context. We present the analysis of ISOCAM-CVF and the J, H, and K-s photometry data for the HII region complex N4 in the Large Magellanic Cloud (LMC). Aims. The aim is twofold: 1) to study the connection between the ...
    • Millimeter dust continuum emission revealing the true mass of giant molecular clouds in the Small Magellanic Cloud 
      Bot, Caroline; Boulanger, Francois; Rubio López, Mónica; Rantakyro, F. (2007)
      Context. CO observations have been the best way so far to trace molecular gas in external galaxies, but in low metallicity environments the gas mass deduced could be largely underestimated due to enhanced photodissociation ...
    • Millimeter dust emission compared with other mass estimates in N11 molecular clouds in the LMC 
      Herrera, C.; Rubio López, Mónica; Bolatto, A.; Boulanger, F.; Israel, F.; Rantakyro, F. (EDP Sciences, 2013)
      CO and dust emission at millimeter wavelengths are independent tracers of cold interstellar matter, which have seldom been compared on the scale of giant molecular clouds (GMCs) in other galaxies. In this study, and for ...
    • Molecular clouds in extreme environments of the low-metallicity magellanic sytem 
      Valdivia Mena, María Teresa (Universidad de Chile, 2020)
      El objetivo de esta tesis es estudiar las propiedades físicas de las nubes moleculares en el Puente de Magallanes A (MagBridgeA), fuente que presenta el mayor exceso de emisión a 870 $\mu$m en estudios con telescopios ...