scispace - formally typeset
Journal ArticleDOI

The evaporation of spherical clouds in a hot gas. I - Classical and saturated mass loss rates

L. L. Cowie, +1 more
- 01 Jan 1977 - 
- Vol. 211, pp 135-146
Reads0
Chats0
About
This article is published in The Astrophysical Journal.The article was published on 1977-01-01. It has received 686 citations till now. The article focuses on the topics: Evaporation & Heat flux.

read more

Citations
More filters
Book

Physics of the Interstellar and Intergalactic Medium

TL;DR: In this paper, a comprehensive and richly illustrated textbook on the astrophysics of the interstellar and intergalactic medium is presented, including the gas and dust, as well as the electromagnetic radiation, cosmic rays, and magnetic and gravitational fields, present between the stars in a galaxy and also between galaxies themselves.
Journal ArticleDOI

What Shapes the Luminosity Function of Galaxies

TL;DR: In this paper, the authors investigate the physical mechanisms that shape the luminosity function of galaxies in hierarchical clustering models and demonstrate that while feedback of form 1 is able to flatten the faint end of the galaxy luminosity, this process alone does not produce the sharp cutoff observed at large luminosities.
Journal ArticleDOI

Cluster Magnetic Fields

TL;DR: Magnetic fields in the intercluster medium have been measured using a variety of techniques, including studies of synchrotron relic and halo radio sources within clusters, studies of inv... as mentioned in this paper.
Journal ArticleDOI

Enzo: an adaptive mesh refinement code for astrophysics

TL;DR: Enzo as discussed by the authors uses block-structured adaptive mesh refinement to provide high spatial and temporal resolution for modeling astrophysical fluid flows, which can be run in one, two, and three dimensions, and supports a wide variety of physics, including hydrodynamics, ideal and non-ideal magnetohydrodynamic, N-body dynamics, primordial gas chemistry, optically thin radiative cooling of primordial and metal-enriched plasmas, and models for star formation and feedback in a cosmological context.
Journal ArticleDOI

Multiphase galaxy formation: high-velocity clouds and the missing baryon problem

TL;DR: In this paper, the authors take into account the expectation that the hot gas in galactic halos is thermally unstable and prone to fragmentation during cooling and show that the implications are more farreaching than previously expected: allowing multi-phase cooling fundamentally alters expectations about gas infall and naturally gives rise to a characteristic upper-limit on the masses of galaxies.
Related Papers (5)