LEADER 03808nam 22006735 450 001 996466689203316 005 20200701144558.0 010 $a3-540-39326-9 024 7 $a10.1007/3-540-15206-7 035 $a(CKB)1000000000230427 035 $a(SSID)ssj0000327023 035 $a(PQKBManifestationID)12089423 035 $a(PQKBTitleCode)TC0000327023 035 $a(PQKBWorkID)10316360 035 $a(PQKB)10609673 035 $a(DE-He213)978-3-540-39326-9 035 $a(PPN)155225936 035 $a(EXLCZ)991000000000230427 100 $a20121227d1985 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt 182 $cc 183 $acr 200 10$aSupernovae as Distance Indicators$b[electronic resource] $eProceedings of a Workshop held at the Harvard-Smithsonian Center for Astrophysics. September 27?28, 1984 /$fedited by Norbert Bartel 205 $a1st ed. 1985. 210 1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d1985. 215 $a1 online resource (VI, 229 p. 12 illus.) 225 1 $aLecture Notes in Physics,$x0075-8450 ;$v224 300 $aBibliographic Level Mode of Issuance: Monograph 311 $a3-540-15206-7 327 $aCurrent problems of determining distances to galaxies -- Multifrequency observations of recent supernovae -- Supernova observations at McDonald observatory -- Spectropolarimetry of supernovae -- Radio emission from a type I supernova -- Radio emission from type II supernovae -- Radio observations of historical, extragalactic supernovae -- Discovery of an entire population of radio supernova candidates in the nucleus of messier 82 -- Detecting supernova remnants in external galaxies -- Diameter determinations of radio supernovae and the distance scale -- Supernove interaction with a circumstellar wind and the distance to SN 1979c -- Model and geometry dependence of radio distance determinations of extragalactic supernovae -- Optical supernovae and the hubble constant -- Type I supernovae as standard candles -- Radius and absolute magnitude of a Cepheid variable -- Astrophysical distances to type II supernovae -- Model atmospheres for type I supernovae -- Accuracy of model parameters from spectroscopic fine analyses of supernovae -- Physical models for type I supernovae and the distance scale -- A preliminary discussion of Hose-Einstein diffusion in supernovae -- Supernovae up close. 410 0$aLecture Notes in Physics,$x0075-8450 ;$v224 606 $aObservations, Astronomical 606 $aAstronomy?Observations 606 $aAstrophysics 606 $aSolid state physics 606 $aSpectroscopy 606 $aMicroscopy 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 606 $aSolid State Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P25013 606 $aSpectroscopy and Microscopy$3https://scigraph.springernature.com/ontologies/product-market-codes/P31090 615 0$aObservations, Astronomical. 615 0$aAstronomy?Observations. 615 0$aAstrophysics. 615 0$aSolid state physics. 615 0$aSpectroscopy. 615 0$aMicroscopy. 615 14$aAstronomy, Observations and Techniques. 615 24$aAstrophysics and Astroparticles. 615 24$aSolid State Physics. 615 24$aSpectroscopy and Microscopy. 676 $a520 702 $aBartel$b Norbert$4edt$4http://id.loc.gov/vocabulary/relators/edt 906 $aBOOK 912 $a996466689203316 996 $aSupernovae as distance indicators$91491079 997 $aUNISA