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Effect of radiation pressure in the cores of globular clusters

Journal Article:

Abstract

The possible effects of a presence of a dust cloud in the cores of globular clusters was investigated. Two cluster models were considered together with various models of clouds. The problem of radiation transfer was solved under some simplifying assumptions. Owing to a differential absorption of the star light in the cloud, radiation pressure turned out be inward-directed in some cloud models. This fact may lead to a confinement of some dust in the central regions of globular clusters.
Publication Date:
Oct 01, 1981
Product Type:
Journal Article
Reference Number:
EDB-82-051538
Resource Relation:
Journal Name: Astron. Astrophys.; (Germany, Federal Republic of); Journal Volume: 102:2
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; STAR CLUSTERS; RADIATION PRESSURE; CLOUDS; COSMIC DUST; RADIANT HEAT TRANSFER; DUSTS; ENERGY TRANSFER; HEAT TRANSFER; 640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources
OSTI ID:
5626206
Country of Origin:
Germany
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: AAEJA
Submitting Site:
DE
Size:
Pages: 250-256
Announcement Date:

Journal Article:

Citation Formats

Angeletti, L, Capuzzo-Dolcetta, R, and Giannone. Effect of radiation pressure in the cores of globular clusters. Germany: N. p., 1981. Web.
Angeletti, L, Capuzzo-Dolcetta, R, & Giannone. Effect of radiation pressure in the cores of globular clusters. Germany.
Angeletti, L, Capuzzo-Dolcetta, R, and Giannone. 1981. "Effect of radiation pressure in the cores of globular clusters." Germany.
@misc{etde_5626206,
title = {Effect of radiation pressure in the cores of globular clusters}
author = {Angeletti, L, Capuzzo-Dolcetta, R, and Giannone}
abstractNote = {The possible effects of a presence of a dust cloud in the cores of globular clusters was investigated. Two cluster models were considered together with various models of clouds. The problem of radiation transfer was solved under some simplifying assumptions. Owing to a differential absorption of the star light in the cloud, radiation pressure turned out be inward-directed in some cloud models. This fact may lead to a confinement of some dust in the central regions of globular clusters.}
journal = {Astron. Astrophys.; (Germany, Federal Republic of)}
volume = {102:2}
journal type = {AC}
place = {Germany}
year = {1981}
month = {Oct}
}