Skip to main content Accessibility help

We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.

Close cookie message
×
  1. Home
  2. Search

Refine search

Refine search

Access:
Content type:
Publication date:
Apply   From and To filters
Subject: Show more
Journals Show more
Publishers: Show more
Societies Show more
Series: Show more
Collections: Show more

Actions for selected content:

Select all | Deselect all
  • View selected items
  • Export citations
  • Download PDF (zip)
  • Save to Kindle
  • Save to Dropbox
  • Save to Google Drive

Save Search

You can save your searches here and later view and run them again in "My saved searches".

Please provide a title, maximum of 40 characters.
Cancel
×

2 results

  • Widths of crossings in Poisson Boolean percolation

  • Part of
  • Ioan Manolescu, Leonardo V. Santoro
  • Journal:
    Journal of Applied Probability , First View
    Published online by Cambridge University Press:
    26 November 2024, pp. 1-25
    • Article
      • You have access
      • Open access
    • PDF
    • HTML
    • Export citation

  • We answer the following question: if the occupied (or vacant) set of a planar Poisson Boolean percolation model contains a crossing of an $n\times n$ square, how wide is this crossing? The answer depends on whether we consider the critical, sub-, or super-critical regime, and is different for the occupied and vacant sets.

  • New axes for the stellar mass fundamental plane

  • Paul L. Schechter
  • Journal:
    Proceedings of the International Astronomical Union / Volume 11 / Issue S317 / August 2015
    Published online by Cambridge University Press:
    09 May 2016, pp. 35-38
    Print publication:
    August 2015
    • Article
      • You have access
    • PDF
    • Export citation

  • We argue that the stellar velocity dispersion observed in an elliptical galaxy is a good proxy for the halo velocity dispersion. As dark matter halos are almost completely characterized by a single scale parameter, the stellar velocity dispersion tells us the virial radius of the halo and the mass contained within. This permits non-dimensionalizing of the stellar mass and effective radius axes of the stellar mass fundamental plane by the virial radius and halo mass, respectively.