Now showing items 1-20 of 37

    • Duronea, N.; Vásquez, J.; Gómez, L.; Cappa, C.; Firpo, V.; López Caraballo, C.; Rubio López, Mónica (EDP Sciences, 2015)
      Aims. We present here a study of the cold dust in the close environs of the ring nebula Gum 31. We aim at deriving the physical properties of the molecular gas and dust associated with the nebula, and investigating its ...
    • Cramer, W. J.; Kenney, J. D. P.; Cortes, J. R.; Cortes, P. C.; Vlahakis, C.; Jáchym, P.; Pompei, E.; Rubio López, Mónica (IOP Publishing, 2020)
      High-resolution (1 '' x 2 '') Atacama Large Millimeter Array CO(2-1) observations of the ram pressure stripped galaxy NGC 4402 in the Virgo cluster show some of the clearest evidence yet for the impacts of ram pressure on ...
    • Valdivia Mena, María Teresa; Rubio López, Mónica; Bolatto, A. D.; Saldaño, H. P.; Verdug, C. (EDP Science, 2020)
      Context. The Magellanic Bridge is a tidal feature located between the Magellanic Clouds, containing young stars formed in situ. Its proximity allows high-resolution studies of molecular gas, dust, and star formation in a ...
    • Ortega, M. E.; Paron, S.; Giacani, E.; Rubio López, Mónica; Dubner, G. (EDP Sciences, 2013-08)
      Aims. We characterize a bright-rimmed cloud embedded in the H II region Sh2-48 while searching for evidence of triggered star formation. Methods. We carried out observations towards a region of 2' x 2' centered at RA ...
    • Elmegreen, Bruce G.; Rubio López, Mónica; Hunter, Deidre A.; Verdugo, Celia; Brinks, Elías; Schruba, Andreas (Macmillan Publishers, 2013)
    • Sorai, K.; Hasegawa, T.; Booth, Roy S.; Rubio López, Mónica; Morino, J. I.; Bronfman Aguiló, Leonardo; Handa, T.; Hatashi, M.; Nyman, L. A.; Oka, T.; Sakamoto, S.; Seta, M.; Usuda, K. S. (2001-04-20)
      We observed 34 positions throughout the disk of the Large Magellanic Cloud in the CO J = 21 emission line with the Tokyo-Onsala-ESO-Calán 60 cm radio telescope. Comparing the spectra with those of the J = 10 line at the ...
    • Rubio López, Mónica; Elmegreen, Bruce G.; Hunter, Deidre A.; Brink, Elias; Cortés, Juan R.; Cigan, Phil (Macmillan, 2015)
      Understanding stellar birth requires observations of the clouds in which they form. These clouds are dense and self-gravitating, and in all existing observations they are molecular, with H2 the dominant species and ...
    • Oey, M. S.; López Hernández, J.; Kellar, J. A.; Pellegrini, E. W.; Gordon, K. D.; Jameson, K. E.; Li, A.; Madden, S. C.; Meixner, M.; Roman Duval, Julia; Bot, C.; Rubio López, Mónica; Tielens, A. G. G. M. (IOP Publishing Ltd, 2017)
      We use the Spitzer Surveying the Agents of Galaxy Evolution (SAGE) survey of the Magellanic Clouds to evaluate the relationship between the 8 mu m polycyclic aromatic hydrocarbon (PAH) emission, 24 mu m hot dust emission, ...
    • Galametz, M.; Hony, S.; Albrecht, M.; Galliano, F.; Cormier, D.; Lebouteiller, V.; Lee, M.; Madden, S.; Bolatto, A.; Bot, C.; Hughes, A.; Israel, F.; Meixner, M.; Oliviera, J.; Paradis, D.; Pellegrini, E.; Roman Duval, Julia; Rubio López, Mónica; Sewilo, M.; Fukui, Y.; Kawamura, A.; Onishi, T. (OXFORD UNIV PRESS, 2016)
      We combine Spitzer and Herschel data of the star-forming region N11 in the Large Magellanic Cloud (LMC) to produce detailed maps of the dust properties in the complex and study their variations with the interstellar-medium ...
    • Roman Duval, Julia; Israel, F. P.; Bolatto, Alberto; Hughes, A.; Leroy, A.; Meixner, M.; Gordon, K.; Madden, S. C.; Paradis, D.; Kawamura, A.; Li, A.; Sauvage, M.; Wong, T.; Bernard, J. P.; Engelbracht, C.; Hony, S.; Kim, S.; Misselt, K.; Okumura, K.; Ott, Jürgen; Panuzzo, P.; Pineda, J. L.; Reach, W. T.; Rubio López, Mónica (2010)
      12CO rotational emission lines and Hi 21 cm emission. This so-called “FIR excess” is especially noticeable near molecular clouds in the LMC, and has usually been interpreted as indicating the presence of a self-shielded ...
    • Guzmán Veloso, Viviana Gabriela (Universidad de ChileCyberDocs, 2010)
    • 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)
    • Jameson, Katherine E.; Bolatto, Alberto D.; Wolfire, Mark; Warren, Steven R.; Herrera Camus, Rodrigo; Croxall, Kevin; Pellegrini, Eric W.; Smith, John David; Rubio López, Mónica; Indebetouw, Remy; Israel, Frank P.; Meixner, Margaret; Roman Duval, Julia; Loon, Jacco Th. van; Muller, Erik; Verdugo, Celia; Zinnecker, Hans; Okada, Yoko (IOP Publishing Ltd, 2018)
      The Small Magellanic Cloud (SMC) provides the only laboratory to study the structure of molecular gas at high resolution and low metallicity. We present results from the Herschel Spectroscopic Survey of the SMC (HS3), which ...
    • Hony, S.; Galliano, F.; Madden, S. C.; Panuzzo, P.; Meixner, M.; Engelbracht, C.; Misselt, K.; Galametz, M.; Sauvage, M.; Roman Duval, Julia; Gordon, K.; Lawton, B.; Bernard, J. P.; Bolatto, Alberto; Okumura, K.; Chen, C.-H. R.; Indebetouw, R.; Israel, F. P.; Kwon, E.; Li, A.; Kemper, F.; Oey, M. S.; Rubio López, Mónica; Triou, H. E. (EDP Sciences, 2010-07)
      Aims. We study the structure of the medium surrounding sites of high-mass star formation to determine the interrelation between the H ii regions and the environment from which they were formed. The density distribution of ...
    • Ortega, M. E.; Paron, S.; Areal, M. B.; Rubio López, Mónica (EDP Sciences, 2020)
      Aims. Cometary globules, dense molecular gas structures exposed to UV radiation, are found inside HII regions. Understanding the nature and origin of these structures through a kinematic study of the molecular gas could ...
    • Bot, Caroline; Rubio López, Mónica; Boulanger, Francois; Albrecht, M.; Leroy, A.; Bolatto, Alberto; Bertoldi, F.; Gordon, K.; Engelbracht, C.; Block, M.; Misselt, K. (2010)
      Context. The amount of molecular gas is a key to understanding the future star formation in a galaxy. Because H2 is difficult to observe directly in dense and cold clouds, tracers such as the CO molecule are used. However, ...
    • Cappa, C.; Duronea, N.; Firpo, V.; Vasquez, J.; López Caraballo, C.; Rubio López, Mónica; Vazzano, M. (EDP SCIENCES, 2015)
      Aims. We present a multi-wavelength analysis of the infrared dust bubble S 24, and the extended IR sources G341.220-0.213 and G341.217-0.237 located in its environs, with the aim of investigating the characteristics of ...
    • Ferrero, Leticia V.; Cappa, Cristina E.; Saldaño, Hugo P.; Gómez, Mercedes; Rubio López, Mónica; Günthardt, Guillermo (Oxford University Press, 2020)
      We present a multiwavelength study of two Herbig-Haro (HH) objects (137 and 138) that may be associated. We use Gemini H-2 (2.12 mu m) and K (2.2 mu m) images, as well as Atacama Pathfinder EXperiment molecular line ...
    • Elmegreen, Bruce G.; Herrera, Cinthya; Rubio López, Mónica; Elmegreen, Debra Meloy; Sánchez Almeida, Jorge; Muñoz-Tuñón, Casiana; Olmo-García, Amanda (Iop Publishing LTD, 2018-06)
      A giant star-forming region in a metal-poor dwarf galaxy has been observed in optical lines with the 10 m Gran Telescopio Canarias (GTC) and in the emission line of CO(1-0) with the Northern Extended Millimeter Array (NOEMA) ...
    • Kalari, Venu M.; Rubio López, Mónica; Elmegreen, Bruce G.; Guzman, Viviana V.; Zinnecker, Hans; Herrera, Cinthya N. (IOP Publishing Ltd, 2018)
      We present new sensitive CO(2-1) observations of the 30 Doradus region in the Large Magellanic Cloud. We identify a chain of three newly discovered molecular clouds that we name KN1, KN2, and KN3 lying within 2-14 pc in ...