Astrophysical: Galaxies

  • Publication
    The [CII] 158 μm emission line as a gas mass tracer in high redshift quiescent galaxies
    A great deal of effort has been made in recent years to probe the gas fraction evolution of massive quiescent galaxies (QGs); however, a clear picture has not...
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    Thermal Instability in a Cooling and Expanding Medium Including Self-Gravity and Conduction
    A systematic study of the linear thermal stability of a medium subject to cooling, self-gravity, and thermal conduction is carried out for the case when the...
  • Publication
    Thick disks and secular evolution
    The detailed study of the different structural components of nearby galaxies can supply vital information about the secular, or internal, evolution of these...
  • Publication
    Thick Disks of Edge-on Galaxies Seen through the Spitzer Survey of Stellar Structure in Galaxies (S4G): Lair of Missing Baryons?
    Most, if not all, disk galaxies have a thin (classical) disk and a thick disk. In most models thick disks are thought to be a necessary consequence of the disk...
  • Publication
    Thick disks of lenticular galaxies. 3D-photometric thin/thick disk decomposition of eight edge-on s0 galaxies
    Thick disks are faint and extended stellar components found around several disk galaxies including our Milky Way. The Milky Way thick disk, the only one studied...
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    Thin discs, thick dwarfs and the effects of stellar feedback
    We investigate the role of stellar mass in shaping the intrinsic thickness of galaxy discs by determining the probability distribution of apparent axial ratios...
  • Publication
    Thin shell formation in radiative shocks. 1: Supernova remnants in low-density media
    This paper explores the onset of thin-shell formation in interstellar shocks associated with supernova explosions. We outline a simple but useful scheme that...
  • Publication
    Third-Order Perturbative Approach to Gravitational Instability: Evolution of Isolated Structures and Environmental Effects
    In an Omega 0 = 1 universe, within the classical Eulerian theory of gravitational instability, the redshift evolution of a peculiar velocity field in a region...
  • Publication
    Three Lyman-α-emitting filaments converging to a massive galaxy group at z = 2.91: discussing the case for cold gas infall
    We have discovered a 300 kpc-wide giant Lyman-α (Lyα) nebula centered on the massive galaxy group RO-1001 at z = 2.91 in the Cosmic Evolution Survey field. Keck...