Accretion processes in star formation:
Our understanding of the formation of stars and planetary systems has changed greatly since the first edition of this book was published. This new edition has been thoroughly updated, and now includes material on molecular clouds, binaries, star clusters and the stellar initial mass function (IMF),...
Saved in:
Main Author: | |
---|---|
Format: | eBook |
Language: | English |
Published: |
Cambridge
Cambridge University Press
2009
|
Edition: | Second edition. |
Series: | Cambridge astrophysics
47 |
Links: | https://doi.org/10.1017/CBO9780511552090 |
Summary: | Our understanding of the formation of stars and planetary systems has changed greatly since the first edition of this book was published. This new edition has been thoroughly updated, and now includes material on molecular clouds, binaries, star clusters and the stellar initial mass function (IMF), disk evolution and planet formation. This book provides a comprehensive picture of the formation of stars and planetary systems, from their beginnings in cold clouds of molecular gas to their emergence as new suns with planet-forming disks. At each stage gravity induces an inward accretion of mass, and this is a central theme for the book. The author brings together current observations, rigorous treatments of the relevant astrophysics, and 150 illustrations, to clarify the sequence of events in star and planet formation. It is a comprehensive account of the underlying physical processes of accretion for graduate students and researchers. |
Physical Description: | 1 Online-Ressource (xiv, 332 Seiten) |
ISBN: | 9780511552090 |
Staff View
MARC
LEADER | 00000nam a2200000 i 4500 | ||
---|---|---|---|
001 | ZDB-20-CTM-CR9780511552090 | ||
003 | UkCbUP | ||
005 | 20151005020622.0 | ||
006 | m|||||o||d|||||||| | ||
007 | cr|||||||||||| | ||
008 | 090512s2009||||enk o ||1 0|eng|d | ||
020 | |a 9780511552090 | ||
100 | 1 | |a Hartmann, Lee |d 1950- | |
245 | 1 | 0 | |a Accretion processes in star formation |c Lee Hartmann |
250 | |a Second edition. | ||
264 | 1 | |a Cambridge |b Cambridge University Press |c 2009 | |
300 | |a 1 Online-Ressource (xiv, 332 Seiten) | ||
336 | |b txt | ||
337 | |b c | ||
338 | |b cr | ||
490 | 1 | |a Cambridge astrophysics |v 47 | |
520 | |a Our understanding of the formation of stars and planetary systems has changed greatly since the first edition of this book was published. This new edition has been thoroughly updated, and now includes material on molecular clouds, binaries, star clusters and the stellar initial mass function (IMF), disk evolution and planet formation. This book provides a comprehensive picture of the formation of stars and planetary systems, from their beginnings in cold clouds of molecular gas to their emergence as new suns with planet-forming disks. At each stage gravity induces an inward accretion of mass, and this is a central theme for the book. The author brings together current observations, rigorous treatments of the relevant astrophysics, and 150 illustrations, to clarify the sequence of events in star and planet formation. It is a comprehensive account of the underlying physical processes of accretion for graduate students and researchers. | ||
776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |z 9780521531993 |
776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |z 9780521825016 |
966 | 4 | 0 | |l DE-91 |p ZDB-20-CTM |q TUM_PDA_CTM |u https://doi.org/10.1017/CBO9780511552090 |3 Volltext |
912 | |a ZDB-20-CTM | ||
912 | |a ZDB-20-CTM | ||
049 | |a DE-91 |
Record in the Search Index
DE-BY-TUM_katkey | ZDB-20-CTM-CR9780511552090 |
---|---|
_version_ | 1832177781578924033 |
adam_text | |
any_adam_object | |
author | Hartmann, Lee 1950- |
author_facet | Hartmann, Lee 1950- |
author_role | |
author_sort | Hartmann, Lee 1950- |
author_variant | l h lh |
building | Verbundindex |
bvnumber | localTUM |
collection | ZDB-20-CTM |
edition | Second edition. |
format | eBook |
fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01771nam a2200277 i 4500</leader><controlfield tag="001">ZDB-20-CTM-CR9780511552090</controlfield><controlfield tag="003">UkCbUP</controlfield><controlfield tag="005">20151005020622.0</controlfield><controlfield tag="006">m|||||o||d||||||||</controlfield><controlfield tag="007">cr||||||||||||</controlfield><controlfield tag="008">090512s2009||||enk o ||1 0|eng|d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9780511552090</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Hartmann, Lee</subfield><subfield code="d">1950-</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Accretion processes in star formation</subfield><subfield code="c">Lee Hartmann</subfield></datafield><datafield tag="250" ind1=" " ind2=" "><subfield code="a">Second edition.</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Cambridge</subfield><subfield code="b">Cambridge University Press</subfield><subfield code="c">2009</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (xiv, 332 Seiten)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield></datafield><datafield tag="490" ind1="1" ind2=" "><subfield code="a">Cambridge astrophysics</subfield><subfield code="v">47</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Our understanding of the formation of stars and planetary systems has changed greatly since the first edition of this book was published. This new edition has been thoroughly updated, and now includes material on molecular clouds, binaries, star clusters and the stellar initial mass function (IMF), disk evolution and planet formation. This book provides a comprehensive picture of the formation of stars and planetary systems, from their beginnings in cold clouds of molecular gas to their emergence as new suns with planet-forming disks. At each stage gravity induces an inward accretion of mass, and this is a central theme for the book. The author brings together current observations, rigorous treatments of the relevant astrophysics, and 150 illustrations, to clarify the sequence of events in star and planet formation. It is a comprehensive account of the underlying physical processes of accretion for graduate students and researchers. </subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe</subfield><subfield code="z">9780521531993</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe</subfield><subfield code="z">9780521825016</subfield></datafield><datafield tag="966" ind1="4" ind2="0"><subfield code="l">DE-91</subfield><subfield code="p">ZDB-20-CTM</subfield><subfield code="q">TUM_PDA_CTM</subfield><subfield code="u">https://doi.org/10.1017/CBO9780511552090</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-20-CTM</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-20-CTM</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-91</subfield></datafield></record></collection> |
id | ZDB-20-CTM-CR9780511552090 |
illustrated | Not Illustrated |
indexdate | 2025-05-15T09:21:33Z |
institution | BVB |
isbn | 9780511552090 |
language | English |
open_access_boolean | |
owner | DE-91 DE-BY-TUM |
owner_facet | DE-91 DE-BY-TUM |
physical | 1 Online-Ressource (xiv, 332 Seiten) |
psigel | ZDB-20-CTM TUM_PDA_CTM ZDB-20-CTM |
publishDate | 2009 |
publishDateSearch | 2009 |
publishDateSort | 2009 |
publisher | Cambridge University Press |
record_format | marc |
series2 | Cambridge astrophysics |
spelling | Hartmann, Lee 1950- Accretion processes in star formation Lee Hartmann Second edition. Cambridge Cambridge University Press 2009 1 Online-Ressource (xiv, 332 Seiten) txt c cr Cambridge astrophysics 47 Our understanding of the formation of stars and planetary systems has changed greatly since the first edition of this book was published. This new edition has been thoroughly updated, and now includes material on molecular clouds, binaries, star clusters and the stellar initial mass function (IMF), disk evolution and planet formation. This book provides a comprehensive picture of the formation of stars and planetary systems, from their beginnings in cold clouds of molecular gas to their emergence as new suns with planet-forming disks. At each stage gravity induces an inward accretion of mass, and this is a central theme for the book. The author brings together current observations, rigorous treatments of the relevant astrophysics, and 150 illustrations, to clarify the sequence of events in star and planet formation. It is a comprehensive account of the underlying physical processes of accretion for graduate students and researchers. Erscheint auch als Druck-Ausgabe 9780521531993 Erscheint auch als Druck-Ausgabe 9780521825016 |
spellingShingle | Hartmann, Lee 1950- Accretion processes in star formation |
title | Accretion processes in star formation |
title_auth | Accretion processes in star formation |
title_exact_search | Accretion processes in star formation |
title_full | Accretion processes in star formation Lee Hartmann |
title_fullStr | Accretion processes in star formation Lee Hartmann |
title_full_unstemmed | Accretion processes in star formation Lee Hartmann |
title_short | Accretion processes in star formation |
title_sort | accretion processes in star formation |
work_keys_str_mv | AT hartmannlee accretionprocessesinstarformation |