Now showing items 1-3 of 3

    • 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 ...
    • 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, ...
    • Villanueva, V.; Bolatto, A.; Vogel, S.; Levy, R. C.; Sánchez, S. F.; Barrera Ballesteros, J.; Wong, T.; Rosolowsky, E.; Colombo, D.; Rubio López, Mónica Solange; Cao, Y.; Kalinova, V.; Leroy, A.; Utomo, D.; Herrera Camus, R.; Blitz, L.; Luo, Y. (IOP, 2021)
      The Astrophysical Journal The American Astronomical Society, find out more The Institute of Physics, find out more The EDGE-CALIFA Survey: The Resolved Star Formation Efficiency and Local Physical Conditions V. ...