LEADER 03647nam 22005775 450 001 996466700103316 005 20200701074644.0 010 $a3-540-48041-2 024 7 $a10.1007/3-540-18653-0 035 $a(CKB)1000000000230696 035 $a(SSID)ssj0000322330 035 $a(PQKBManifestationID)12133578 035 $a(PQKBTitleCode)TC0000322330 035 $a(PQKBWorkID)10287579 035 $a(PQKB)11292017 035 $a(DE-He213)978-3-540-48041-9 035 $a(PPN)155232592 035 $a(EXLCZ)991000000000230696 100 $a20121227d1987 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt 182 $cc 183 $acr 200 10$aCool Stars, Stellar Systems, and the Sun$b[electronic resource] $eProceedings of the Fifth Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun Held in Boulder, Colorado, July 7?11, 1987 /$fedited by Jeffrey L. Linsky, Robert E. Stencel 205 $a1st ed. 1987. 210 1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d1987. 215 $a1 online resource (XIII, 538 p. 45 illus.) 225 1 $aLecture Notes in Physics,$x0075-8450 ;$v291 300 $aBibliographic Level Mode of Issuance: Monograph 311 $a3-540-18653-0 327 $aContents: Stellar Magnetic Fields -- Nonthermal Phenomena in Stellar Coronae -- Heating of Stellar Chromospheres and Coronae -- The Angular Momentum History of Stars -- Stars with Thin and Thick Convective Zones -- Re-examining the Corona/Wind Dividing Line -- Exploiting the Infrared -- Activity in Pre-Main Sequence Stars -- Panel on Monitoring Programs -- Contributed Papers on Active Binary Stars -- Author Index. 330 $aRecent research on the solar-stellar system has been triggered by a host of recent observational data, in particular from space based observations. For this conference the major topics selected centered on new measurement capabilities (magnetic fields and infrared, with specific emphasis on the new IRAS results), important classes of stars (F stars, M dwarfs and giants, and pre-main sequence stars), and interesting unanswered questions (the nature of nonthermal phenomena, heating processes, angular momentum evolution, and the existence and cause of the corona/wind dividing line). Each section is opened by two or more invited lectures aimed at a wide audience, including graduate students, and continues with some research papers. The proceedings also record the two general discussions on the role of magnetic fields in cool star atmospheres and the role of monitoring programs for studies of cool stars (see also Lecture Notes in Physics Vol. 292). 410 0$aLecture Notes in Physics,$x0075-8450 ;$v291 606 $aObservations, Astronomical 606 $aAstronomy?Observations 606 $aAstrophysics 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 615 0$aObservations, Astronomical. 615 0$aAstronomy?Observations. 615 0$aAstrophysics. 615 14$aAstronomy, Observations and Techniques. 615 24$aAstrophysics and Astroparticles. 676 $a520 702 $aLinsky$b Jeffrey L$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aStencel$b Robert E$4edt$4http://id.loc.gov/vocabulary/relators/edt 906 $aBOOK 912 $a996466700103316 996 $aCool stars, stellar systems, and the sun$91118139 997 $aUNISA