Publication type: Non-refereed

  • Publication
    Models of solar magnetic structures (Socas-Navarro, 2007)
    The observations used in this work were acquired with the new Spectro-Polarimeter for Infrared and Optical Regions (SPINOR; Socas-Navarro et al., 2006SoPh..235...
  • Publication
    Modified Newtonian Dynamics, an Introductory Review
    By the time, in 1937, the Swiss astronomer Zwicky measured the velocity dispersion of the Coma cluster of galaxies, astronomers somehow got acquainted with the...
  • Publication
    Molar extinction coefficient of fullerenes and related hydrogenated derivatives ``fulleranes''
    Fullerenes, the carbon molecules with 60 and 70 atoms, were recently detected in a series of planetary nebulae, in protoplanetary nebulae and in other...
  • Publication
    Molecolar hydrogen knots in Chamaeleon I dark cloud
    We have searched for shock-excited molecular hydrogen knots in five selected areas of the Chamaeleon I dark cloud using narrow-band images centered on the H_2...
  • Publication
    Molecular Gas and Dust in the Brightest Cluster Galaxy of MACS 1931.8-2635
    We present the results of band 3, 6, and 7 ALMA observations obtained of the brightest cluster galaxy (BCG) in MACS 1931.8-2635 over the course of Cycles 4 and...
  • Publication
    Molecular gas in galaxies, and evolution with redshift
    Not Available
  • Publication
    Molecular gas in star-forming galaxies of the intermediate redshift cluster Zw Cl0024
    We present preliminary results from a survey of cold gas in an intermediate-redshift cluster, Zw Cl0024.1+1652 at z = 0.395, using the EMIR receiver at the IRAM...
  • Publication
    Molecular gas in/outflows in the nuclear regions of five Seyfert galaxies
    One of the most challenging open questions in Astrophysics is how Active Galactic Nuclei (AGNs) are fueled. For this to happen, gas has to be driven from the...
  • Publication
    Molecular Hydrogen Around Post-AGB Stars
    Near-infrared spectroscopy was conducted to search for molecular material around 40 post-AGB stars. We present the detection of molecular emission lines of H2...