| Record ID | harvard_bibliographic_metadata/ab.bib.13.20150123.full.mrc:942283120:2057 |
| Source | Harvard University |
| Download Link | /show-records/harvard_bibliographic_metadata/ab.bib.13.20150123.full.mrc:942283120:2057?format=raw |
LEADER: 02057nam a22004335a 4500
001 013832867-6
005 20131206194903.0
008 130616s1995 gw | s ||0| 0|eng d
020 $a9783540492177
020 $a9783540492177
020 $a9783662224823
024 7 $a10.1007/978-3-540-49217-7$2doi
035 $a(Springer)9783540492177
040 $aSpringer
050 4 $aQB4
072 7 $aPG$2bicssc
072 7 $aSCI004000$2bisacsh
072 7 $aNAT033000$2bisacsh
082 04 $a520$223
100 1 $aTinney, Christopher G.,$eeditor.
245 14 $aThe Bottom of the Main Sequence — And Beyond :$bProceedings of the ESO Workshop Held in Garching, Germany, 10–12 August 1994 /$cedited by Christopher G. Tinney.
264 1 $aBerlin, Heidelberg :$bSpringer Berlin Heidelberg :$bImprint: Springer,$c1995.
300 $aXVII, 309 p.$bonline resource.
336 $atext$btxt$2rdacontent
337 $acomputer$bc$2rdamedia
338 $aonline resource$bcr$2rdacarrier
347 $atext file$bPDF$2rda
490 1 $aESO Astrophysics Symposia, European Southern Observatory,$x1431-2433
520 $aThis is a complete overview of the state of the art in the study of very-low-mass stars, particularly brown dwarfs. It covers observations as well as modelling techniques, especially addressing the current status of our theoretical understanding of these objects, and the relation of observed luminosity and mass functions to star formation. Besides the problems of clustering, surface activity, and current estimates of the mass density in low-mass stars, the reader will also learn how many bona fide brown dwarfs have been unambigously detected so far.
650 10 $aPhysics.
650 0 $aPhysics.
650 0 $aPhysical geography.
650 24 $aAstronomy, Observations and Techniques.
650 24 $aAstrophysics and Astroparticles.
650 24 $aGeophysics/Geodesy.
776 08 $iPrinted edition:$z9783662224823
830 0 $aESO Astrophysics Symposia, European Southern Observatory.
988 $a20131114
906 $0VEN