Astrophysical: Star formation

  • Publication
    Star formation and gas in the minor merger UGC 10214
    Minor mergers play a crucial role in galaxy evolution. UGC 10214 (the Tadpole galaxy) is a prime example of this process in which a dwarf galaxy has interacted...
  • Publication
    Star formation and gas in the minor merger UGC 10214 (Corrigendum)
  • Talk
    Star formation driven by cold-flow accretion in the local Universe
    The direct accretion of pristine gas streams is predicted to be the main mode of galaxy disk growth in the early universe (cold-flows). We (think we) have...
  • Publication
    Star formation efficiency patterns in the spiral arms of M51
    The distribution of ionized, molecular, and atomic hydrogen in the disk and especially along the spiral arms of the Whirlpool galaxy, M51, is investigated by...
  • Publication
    Star Formation Histories of Ultra-faint Dwarf Galaxies: Environmental Differences between Magellanic and Non-Magellanic Satellites?
    We present the color-magnitude diagrams and star formation histories (SFHs) of seven ultra-faint dwarf galaxies: Horologium 1, Hydra 2, Phoenix 2, Reticulum 2...
  • Publication
    Star formation history for the starburst dwarf galaxy in the Local Group, IC 10
    IC 10 as a starburst dwarf galaxy in the Local Group (LG) has a large population of newly formed stars that are massive and intrinsically very bright in...
  • Publication
    Star Formation History of Two Fields in the Halo of NGC 5128
    NGC 5128 galaxy is a giant elliptical galaxy located in the Centaurus group of galaxies at 3.8 Mpc. We aim to study the star formation history (SFH) of two...
  • Publication
    Star formation in outer rings of S0 galaxies. V. UGC 4599: An S0 with gas probably accreted from a filament
    Aims: Though S0 galaxies are usually thought to be `red and dead', they often demonstrate weak star formation organised in ring structures and located in their...
  • Publication
    Star formation in Seyfert galaxies
    An analysis of the IRAS data for a sample of classical (optically selected) Seyfert galaxies is presented. The IRAS fluxes at 25 micron, 60 micron, and 100...