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Stellar Pulsations (Record no. 27059)

000 -LEADER
fixed length control field 02730nam a22004575i 4500
003 - CONTROL NUMBER IDENTIFIER
control field OSt
005 - DATE AND TIME OF LATEST TRANSACTION
control field 20140310153037.0
007 - PHYSICAL DESCRIPTION FIXED FIELD--GENERAL INFORMATION
fixed length control field cr nn 008mamaa
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION
fixed length control field 121026s2013 gw | s |||| 0|eng d
020 ## - INTERNATIONAL STANDARD BOOK NUMBER
International Standard Book Number 9783642296307
978-3-642-29630-7
050 #4 - LIBRARY OF CONGRESS CALL NUMBER
Classification number QB1-991
Classification number QB460-466
Classification number QB980-991
082 04 - DEWEY DECIMAL CLASSIFICATION NUMBER
Classification number 520
Edition number 23
264 #1 -
-- Berlin, Heidelberg :
-- Springer Berlin Heidelberg :
-- Imprint: Springer,
-- 2013.
912 ## -
-- ZDB-2-PHA
100 1# - MAIN ENTRY--PERSONAL NAME
Personal name Suárez, J.C.
Relator term editor.
245 10 - IMMEDIATE SOURCE OF ACQUISITION NOTE
Title Stellar Pulsations
Medium [electronic resource] :
Remainder of title Impact of New Instrumentation and New Insights /
Statement of responsibility, etc edited by J.C. Suárez, R. Garrido, L. A. Balona, J. Christensen-Dalsgaard.
300 ## - PHYSICAL DESCRIPTION
Extent XVII, 293 p. 79 illus.
Other physical details online resource.
440 1# - SERIES STATEMENT/ADDED ENTRY--TITLE
Title Astrophysics and Space Science Proceedings,
International Standard Serial Number 1570-6591 ;
Volume number/sequential designation 31
505 0# - FORMATTED CONTENTS NOTE
Formatted contents note Part I Oral Contributions -- 1 The poor agreement between observed & predicted frequencies -- 2 Giant Stars -- 3 New instrumentation from the ground & space -- 4 Mode identification -- 5 Oscillations versus activity plus planet transits -- 6 Early type stars. Oscillations versus other agents, mainly regular/rotational variations of B stars -- 7 Conference closing remarks -- Part II Poster Contributions -- 8 List of poster contributions.
520 ## - SUMMARY, ETC.
Summary, etc Analyses of photometric time series obtained from the MOST, CoRoT and Kepler space missions were presented at the 20th conference on Stellar Pulsations (Granada, September 2011). These results are leading to a re-appraisal of our views on stellar pulsation in some stars and posing some new and unexpected challenges. The very important and exciting role played by innovative ground-based observational techniques, such as interferometric measurements of giant pulsating stars and high-resolution spectroscopy in the near infrared, is also discussed. These Proceedings are distinguished by the format of the conference, which brings together a variety of related but different topics not found in other meetings of this nature.
650 #0 - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name as entry element Physics.
Topical term or geographic name as entry element Astronomy.
Topical term or geographic name as entry element Physics.
Topical term or geographic name as entry element Astronomy, Astrophysics and Cosmology.
700 1# - ADDED ENTRY--PERSONAL NAME
Personal name Garrido, R.
Relator term editor.
Personal name Balona, L. A.
Relator term editor.
Personal name Christensen-Dalsgaard, J.
Relator term editor.
710 2# - ADDED ENTRY--CORPORATE NAME
Corporate name or jurisdiction name as entry element SpringerLink (Online service)
773 0# - HOST ITEM ENTRY
Title Springer eBooks
776 08 - ADDITIONAL PHYSICAL FORM ENTRY
Display text Printed edition:
International Standard Book Number 9783642296291
856 40 - ELECTRONIC LOCATION AND ACCESS
Uniform Resource Identifier http://dx.doi.org/10.1007/978-3-642-29630-7
942 ## - ADDED ENTRY ELEMENTS (KOHA)
Source of classification or shelving scheme
Item type E-Book
Copies
Price effective from Permanent location Date last seen Not for loan Date acquired Source of classification or shelving scheme Koha item type Damaged status Lost status Withdrawn status Current location Full call number
2014-04-23AUM Main Library2014-04-23 2014-04-23 E-Book   AUM Main Library520

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