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ورود / ثبت نام
عنوان
Jets from young stars II : clues from high angular resolution observations
پدید آورنده
Francesca Bacciotti, Emma Whelan, Leonardo Testi, )eds.(
موضوع
Observations -- Congresses ، Astrophysical jets,Observations -- Congresses ، Circumstellar matter,Observations -- Congresses ، Stars -- Formation
رده
QC
3
.
L28
Vol
.
742
کتابخانه
Library of Institute for Research in Fundamental Sciences
محل استقرار
استان:
Tehran
ـ شهر:
Tehran
تماس با کتابخانه :
22291812
-
021
TITLE AND STATEMENT OF RESPONSIBILITY
Title Proper
Jets from young stars II : clues from high angular resolution observations
EDITION STATEMENT
Statement of Responsibility Relating to Edition
2006 : Marciana Marina, Italy
.PUBLICATION, DISTRIBUTION, ETC
Place of Publication, Distribution, etc.
Berlin
Name of Publisher, Distributor, etc.
Springer-Verlag
Date of Publication, Distribution, etc.
c2008
PHYSICAL DESCRIPTION
Specific Material Designation and Extent of Item
xii, 291 p.: ill
SERIES
Other Title Information
Lecture notes in physics; 247
GENERAL NOTES
Text of Note
"Second JETSET school on Jets from Young Stars : Clues from High Angular Resolution Observations"-- P. ]4[ of cover
Text of Note
"Second JETSET school....was held at Marciana Marina, Elba Island, Italy, in September 2006"
Text of Note
Includes bibliographies
Text of Note
ISBN: 3540680314
NOTES PERTAINING TO TITLE AND STATEMENT OF RESPONSIBILITY
Text of Note
Francesca Bacciotti, Emma Whelan, Leonardo Testi, )eds.(
ORIGINAL VERSION NOTE
Text of Note
1
TOPICAL NAME USED AS SUBJECT
Entry Element
Observations -- Congresses ، Astrophysical jets
Entry Element
Observations -- Congresses ، Circumstellar matter
Entry Element
Observations -- Congresses ، Stars -- Formation
LIBRARY OF CONGRESS CLASSIFICATION
Class number
QC
3
.
L28
Vol
.
742
PERSONAL NAME - PRIMARY RESPONSIBILITY
Relator Code
AU
AU Bacciotti, Francesca
AU Whelan, Emma
AU Testi, Leonardo
CO Jet Simulations, Experiments and Theory
TI
SE
CORPORATE BODY NAME - PRIMARY RESPONSIBILITY
Entry Element
JETSET School on Jets from Young Stars : Clues from High Angular Resolution Observations
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