Clumping in Hot-star Winds

Clumping in Hot-star Winds
Author :
Publisher : Universitätsverlag Potsdam
Total Pages : 262
Release :
ISBN-10 : 9783940793331
ISBN-13 : 3940793337
Rating : 4/5 (337 Downloads)

Book Synopsis Clumping in Hot-star Winds by : Wolf-Rainer Hamann

Download or read book Clumping in Hot-star Winds written by Wolf-Rainer Hamann and published by Universitätsverlag Potsdam. This book was released on 2008 with total page 262 pages. Available in PDF, EPUB and Kindle. Book excerpt:


Clumping in Hot-star Winds Related Books

Clumping in Hot-star Winds
Language: en
Pages: 262
Authors: Wolf-Rainer Hamann
Categories: Stellar winds
Type: BOOK - Published: 2008 - Publisher: Universitätsverlag Potsdam

DOWNLOAD EBOOK

Instability and Variability of Hot-Star Winds
Language: en
Pages: 475
Authors: Anthony F.J. Moffat
Categories: Science
Type: BOOK - Published: 2012-12-06 - Publisher: Springer Science & Business Media

DOWNLOAD EBOOK

This specialized workshop was conceived during the workshop on "Non isotropic and Variable Outflows from Stars", which was held at the Space Telescope Science I
Very Massive Stars in the Local Universe
Language: en
Pages: 277
Authors: Jorick S. Vink
Categories: Science
Type: BOOK - Published: 2014-10-25 - Publisher: Springer

DOWNLOAD EBOOK

This book presents the status of research on very massive stars in the Universe. While it has been claimed that stars with over 100 solar masses existed in the
Disc Winds Matter
Language: en
Pages: 243
Authors: James Matthews
Categories: Science
Type: BOOK - Published: 2017-08-01 - Publisher: Springer

DOWNLOAD EBOOK

This thesis describes the application of a Monte Carlo radiative transfer code to accretion disc winds in two types of systems spanning 9 orders of magnitude in
Kinematics and Dynamics of Diffuse Astrophysical Media
Language: en
Pages: 388
Authors: John E. Dyson
Categories: Science
Type: BOOK - Published: 2012-12-06 - Publisher: Springer Science & Business Media

DOWNLOAD EBOOK

The area of diffuse astrophysical media is enormous and ranges over circum stellar to extragalactic scales. The physical conditions can vary from cool dusty gas