Penetrating Bars through Masks of Cosmic Dust
By D. Block, Ivanio Puerari, Kenneth C. Freeman, R. Groess, Elizabeth K. Block. 2004
223 citations recorded by the source corpus.
Subfields: Computational Mechanics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/9c52eb2bd96b696896fcc45f44e6b40de00478c4
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Computational Mechanics
- Astronomy
- U. D. O. Physics
- R. Genzel
- D. Ward-Thompson
- Roger Davies
- Peter J. Teuben
- J. Kormendy
- A. Sternberg
In Statistical and Nonlinear Physics
- J. Kormendy
- Alister W. Graham
- N. Drory
- R. Genzel
- Christopher J. Conselice
- R. Bender
- L. Tacconi
- S. Driver
Citations in the corpus
- A Close Look at Star Formation around Active Galactic Nuclei (2007, background): “The global Schmidt law, as formulated by Kennicutt (1998), states that the star formation rate depends on the gas surface density as SFR / 1:4gas.”
- Total Galaxy Magnitudes and Effective Radii from Petrosian Magnitudes and Radii (2005, background): “Things are better for profiles with smaller values of n and if one considers the profiles truncate at 5Re (Figure 2b).”
- BULGELESS GIANT GALAXIES CHALLENGE OUR PICTURE OF GALAXY FORMATION BY HIERARCHICAL CLUSTERING, (2010, background): “2009 is a very incomplete list), and by reviewers (e. g., Burkert & D’Onghia 2004; Lake 2004; Brooks 2010; Peebles & Nusser 2010).”
- The structure of galactic disks - Studying late-type spiral galaxies using SDSS (2006, methodology): “We have used the profiles of three face-on Sbc–Sc galaxies from Pohlen et al. (2002), from which UGC 9837 is also part of our sample.”
- A CLASSICAL MORPHOLOGICAL ANALYSIS OF GALAXIES IN THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G) (2015, unknown): “Detailed observations and numerical simulations (e.g., Bureau & Freeman 1999; Athanassoula & Bureau 1999; Bureau et al. 2004, 2006) have definitively shown that X-structures are related to the edge-on view of a bar.”
- Secular Evolution via Bar-driven Gas Inflow: Results from BIMA SONG (2005, background): “values vary from 14-22 Mpc, assumed 18 Mpc as mid-point value; ap:Block et al. (1999); aq:Karachentsev et al.”
- A 100 pc ELLIPTICAL AND TWISTED RING OF COLD AND DENSE MOLECULAR CLOUDS REVEALED BY HERSCHEL AROUND THE GALACTIC CENTER (2011, background): “The CMZ may be a Galactic analog of the nuclear star-forming rings observed in the centers of star forming barred galaxies (Kormendy & Kennicutt 2004, Kormendy & Cornell 2004).”
- Antitruncation of Disks in Early-Type Barred Galaxies (2005, background): “Pohlen et al. (2002), using very deep exposures of three face-on Sbc–Sc galaxies, showed that truncations can be clearly identified in face-on disks, and that the decline in surface brightness outside the truncation break is best described by an exponential, steeper by about a factor of two than tha”