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· 분류 : 외국도서 > 과학/수학/생태 > 과학 > 천문학
· ISBN : 9780792351528
· 쪽수 : 530쪽
· 출판일 : 1998-08-31
목차
I: Young Stars.- Relation Between Stellar Evolution and Circumstellar Processes (Invited).- Protostars and Protoplanetary Disks (Invited).- ISO Observations of Isolated Herbig AE/BE Stars.- The Intermittently Embedded Herbig AE/BE Stars.- The ISO Spectrum of the Young Star HD 100546.- Far-Infrared Photometry of Circumstellar Matter Around Intermediate Mass Stars.- The ISO Spectrum of the Cloud Core M17-North.- ISO-SWS Observations of Weak Bands of Trace Components of Ices Towards the Young Stellar Object W 33A.- Absorption Features of Ices Toward NGC75381RS1.- PDRS and Shocks in S106 IR and CEP A East.- Search for H2 Emission from Disks Around T Tauri and Herbig AE Stars.- Evolution of Southern Star-Forming Regions.- Dust Disks Around Main Sequence Stars (Invited).- Vega-Like Stars: Grain Removal Replenishment and Recent ISO Observations (Invited).- Dust Around Solar Mass Stars.- Calibration of the Debris Project Isophot Data.- Isophot Observations of VEGA and VEGA-Like Stars.- Isophot S Observations of 3 M Dwarfs.- II: Massive Stars.- Ionized Outflows of Hot Stars (Invited).- Isophot Observations of Early-Type Stars.- HI Infrared Line Formation in Early B-Type Stars.- Transonic Decretion Discs around BE Stars.- ISO's View on Massive Star Evolution: Neon Abundances in Wolf-Rayet Stars (Invited).- ISO SWS Spectroscopy of WR 146 (WC6+0).- ISO Observations of Wolf-Rayet Dust Shells.- Clues to the Evolution of Massive Stars from Their Far-Infrared Environments.- Dust in LBV Nebulae.- Infrared Properties of a Large Ring Around the LBV G79.29+0.46.- ISOCAM Imaging of LBVS.- V 439 CYG as a Late Phase of Stellar Evolution.- Infrared Observations of High-Mass X-Ray Binaries.- ISOCAM Observations of CYG X-3: Search for a Hot Stellar Wind.- First Results from ISO Spectra of Supernova Remnants Heavily Interacting with the ISM (Invited).- ISO Observations of Freshly Synthesized Supernova Material (Invited).- ISO Observations of Classical Novae (Invited).- ISOPHOT Observations of the RS CVN-Type Star HR 7428.- III: Late Stages Of Stellar Evolution.- Molecules in Stellar Atmospheres (Invited).- SO-SWS Spectral Characterization of Stars.- Molecular Features in ISO-SWS Spectra of O-Rich Long-Period Variables.- Dust Formation and Mass Loss in Evolved Stars (Invited).- Theory of AGB Evolution (Invited).- Dramatic Change in Sakurai' s Object.- Model Atmospheres of AGB Stars: Dynamics, Molecules and Dust.- Synthetic Spectra for Carbon Stars from Dynamical Model Atmospheres.- Episodic Mass Loss and Rapid Lithium Enrichment and Depletion in K Giants.- Molecules of Non-Photospheric Origin in Red Giants and Supergiants Revealed by the ISO SWS.- Infrared Emissions from Metals in Carbon Stars and M Giant.- Tentative Detection of Circumstellar CO2 From the AGB Star R Crateris.- Molecules in AGB Stars Observed with ISO (Invited).- ISO LWS Observations of Cool Evolved Stars and Post-AGB Objects (Invited).- ISO LWS Observations of H2O from R Cas: A Consistent Model for Its Circumstellar Envelope.- Excitation of Far-Infrared Lines of OH and Maser Pumping Efficiency in Circumstellar Envelopes.- ISO-SWS Observations of the Time Variability of Oxygen-Rich Mira Variables.- OSO-SWS Spectra of OH/IR Stars.- Isophot Mapping Observations of Carbon Stars.- Isophot Mapping Observations of a Mira-Type AGB Star R Hya.- Spectroscopic Study of Carbon Stars with the ISO-SWS.- ISO-SWS Spectra of Carbon Stars: Molecular Features and a Comparison with Models.- ISO Observations of Symbiotic Stars.- ISO Spectra of Symbiotic Stars.- Analysis of Infrared Spectra of Carbon Stars Observed by the ISO SWS.- ISO-SWS Observations of Stars with Unusual Iras LRS Characteristics.- AGB Stars in the Magellanic Clouds (Invited).- ISO Spectroscopy of AGB Stars in the Magellanic Clouds.- Evolution and Mass Loss of AGB Stars in the Small Magellanic Cloud.- AGB Stars and Supergiants in the Bar of the LMC.- Obscured AGB Stars in the LMC.- The Red Supergiant IRAS04553-6825 in the LMC.- Extreme














