Gas and Galaxy Evolution
By J. Hibbard, M. Rupen, J. Gorkom. 2001
234 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/26b4afe84191914e6b5c6725b7f8613c8aad419b
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
Citations in the corpus
- A Probable z ~ 7 Galaxy Strongly Lensed by the Rich Cluster A2218: Exploring the Dark Ages (2004, unknown): “2 Observatoire Midi-Pyrénées, UMR5572, 14 Avenue Edouard Belin, 31000 Toulouse, France.”
- SIMULATION OF THE COSMIC EVOLUTION OF ATOMIC AND MOLECULAR HYDROGEN IN GALAXIES (2009, methodology): “In fact, we deliberately did not adjust ξ to match the observed HI-mass–HI-radius relation of Verheijen (2001), in order to check the reliability of our models against this observation.”
- Thick gas discs in faint dwarf galaxies (2010, background): “On the other hand, the star formation rate is∼ 10−3 M⊙/yr (Roychowdhury et al. 2009), for which the expected supernova rate for a Salpeter IMF is ∼ 7 × 10−6/yr (Binney 2001).”
- The Central Mass Distribution in Dwarf and Low Surface Brightness Galaxies (2002, background): “On the one hand, there are studies that find that dwarf and LSB galaxies may have steep inner slopes (Swaters 2001b; Pickering et al., in preparation), and on the other hand there are several studies that find that these galaxies are not consistent with steep inner slopes (Borriell & Salucci 2001;…”
- Nuclear Activity in Nearby Galaxies (2008, background): “…Greene & Ho 2006) has generated intense interest in linking BH growth with galaxy formation, as attested by the increasing number of conferences focusing on this theme (e.g., Schmitt, Kinney & Ho 1999; Ho 2004a; Storchi-Bergmann, Ho & Schmitt 2004; Merloni, Nayakshin & Sunyaev 2005; Fiore 2006).”