000 07081nam a22004098i 4500
001 CR9780511552090
003 UkCbUP
005 20200124160232.0
006 m|||||o||d||||||||
007 cr||||||||||||
008 090512s2009||||enk o ||1 0|eng|d
020 _a9780511552090 (ebook)
020 _z9780521825016 (hardback)
020 _z9780521531993 (paperback)
040 _aUkCbUP
_beng
_erda
_cUkCbUP
050 0 0 _aQB806
_b.H39 2009
082 0 0 _a523.8/8
_222
100 1 _aHartmann, Lee,
_d1950-
_eauthor.
245 1 0 _aAccretion processes in star formation /
_cLee Hartmann.
250 _aSecond edition.
264 1 _aCambridge :
_bCambridge University Press,
_c2009.
300 _a1 online resource (xiv, 332 pages) :
_bdigital, PDF file(s).
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
490 1 _aCambridge astrophysics ;
_v47
500 _aTitle from publisher's bibliographic system (viewed on 05 Oct 2015).
505 0 0 _g1.1
_tMolecular clouds
_g2 --
_g1.2
_tThe IMF, clusters, and binaries
_g4 --
_g1.3
_tYoung stars
_g5 --
_g1.4
_tProtostars
_g9 --
_g1.5
_tLong-wavelength emission: dusty envelopes and disks
_g10 --
_g1.6
_tImaging of disks
_g12 --
_g1.7
_tDisk accretion
_g14 --
_g1.8
_tDisks and planet formation
_g16 --
_g1.9
_tA picture of star and planet formation
_g18 --
_g2
_tBeginnings: molecular clouds
_g21 --
_g2.1
_tLarge-scale properties of molecular clouds
_g21 --
_g2.2
_tTurbulence and cloud lifetimes
_g23 --
_g2.3
_tMolecular cloud formation and dispersal
_g26 --
_g2.4
_tFlows, magnetic fields, and cloud formation
_g30 --
_g2.5
_tGravity and fragmentation
_g32 --
_g2.6
_tSheets and filaments
_g34 --
_g2.7
_tTurbulence and cloud structure
_g40 --
_g3
_tInitial conditions for protostellar collapse
_g43 --
_g3.1
_tMolecular cloud cores
_g43 --
_g3.2
_tVirial theorem and cloud stability
_g46 --
_g3.3
_tCentrally concentrated clouds
_g49 --
_g3.4
_tCore lifetimes and equilibrium
_g53 --
_g3.5
_tStability of magnetized clouds
_g54 --
_g3.6
_tAmbipolar diffusion of magnetic flux
_g55 --
_g3.7
_tThe magnetic flux "problem(s)"
_g57 --
_g4
_tProtostellar cloud collapse
_g60 --
_g4.1
_tFree-fall collapse of a uniform cloud
_g60 --
_g4.2
_tSimilarity solution for collapse
_g61 --
_g4.3
_tGeneralized models of protostellar collapse
_g65 --
_g4.4
_tRotating collapse
_g68 --
_g4.5
_tTime evolution of rotating collapse
_g73 --
_g4.6
_tDisk formation
_g74 --
_g4.7
_tMassive protostars
_g76 --
_g5
_tProtostellar collapse: observations vs. theory
_g82 --
_g5.1
_tProtostellar luminosities and accretion
_g84 --
_g5.2
_tSEDs of spherical infalling envelopes
_g86 --
_g5.3
_tSEDs for rotating collapse models
_g91 --
_g5.4
_tA case study: L1551 IRS 5
_g94 --
_g5.5
_tThe Class 0 sources
_g98 --
_g5.6
_tFlat spectrum sources
_g100 --
_g5.7
_tSpatial distribution of emission
_g103 --
_g5.8
_tDetection of infall from line profiles
_g104 --
_g5.9
_tMassive protostars
_g108 --
_g6
_tBinaries, clusters, and the IMF
_g112 --
_g6.1
_tObservations of binary and multiple systems
_g113 --
_g6.2
_tTheories of multiple stellar system formation
_g115 --
_g6.3
_tEvolution of multiple systems during accretion
_g116 --
_g6.4
_tYoung clusters
_g118 --
_g6.5
_tCluster formation
_g121 --
_g6.6
_tThe Initial Mass Function
_g123 --
_g6.7
_tTheories of the IMF
_g125 --
_g7
_tDisk accretion
_g129 --
_g7.1
_tEnergy minimization and angular momentum conservation
_g130 --
_g7.2
_tThe thin accretion disk
_g132 --
_g7.3
_tThe steady optically thick disk
_g139 --
_g7.4
_tThe [alpha] disk
_g142 --
_g7.5
_tSources of viscosity: the magnetorotational instability
_g143 --
_g7.6
_tThe ionization problem
_g146 --
_g7.7
_tGravitational instability and angular momentum transport
_g148 --
_g7.8
_tDisk boundary layers
_g152 --
_g7.9
_tDisk irradiation
_g155 --
_g8
_tThe disks of pre-main-sequence stars
_g158 --
_g8.1
_tDisk imaging
_g161 --
_g8.2
_tDisk SEDs
_g163 --
_g8.3
_tLong-wavelength emission and disk masses
_g168 --
_g8.4
_tDisk/magnetosphere accretion
_g173 --
_g8.5
_tAccretion rates
_g177 --
_g8.6
_tWhat drives accretion?
_g180 --
_g8.7
_tThe WTTS
_g183 --
_g8.8
_tThe Herbig Ae/Be stars
_g184 --
_g8.9
_tThe transitional disks
_g185 --
_g9
_tThe FU Orionis objects
_g188 --
_g9.1
_tBasic observational properties
_g189 --
_g9.2
_tThe accretion disk model
_g192 --
_g9.3
_tDisk kinematics
_g196 --
_g9.4
_tDisk properties
_g200 --
_g9.5
_tTime variability and circumstellar envelopes
_g203 --
_g9.6
_tOutburst mechanisms
_g205 --
_g9.7
_tThe boundary layer problem
_g210 --
_g9.8
_tOutburst statistics and evolutionary significance
_g211 --
_g10
_tDisk winds, jets, and magnetospheric accretion
_g213 --
_g10.1
_tOutflows and jets
_g213 --
_g10.2
_tP Cygni profiles
_g216 --
_g10.3
_tFU Ori disk winds
_g219 --
_g10.4
_tT Tauri winds
_g222 --
_g10.5
_tMass loss rates
_g223 --
_g10.6
_tMagnetocentrifugal acceleration and collimation
_g228 --
_g10.7
_tMagnetohydrodynamic flows
_g229 --
_g10.8
_tMHD disk winds
_g233 --
_g10.9
_tApplications of MHD disk wind theory
_g237 --
_g10.10
_tModels of magnetospheric accretion
_g240 --
_g11
_tDisk accretion and early stellar evolution
_g247 --
_g11.1
_tPre-main-sequence stellar evolutionary tracks
_g247 --
_g11.2
_tProtostellar properties
_g252 --
_g11.3
_tThe "birthline"
_g253 --
_g11.4
_tBirthlines: comparison with observations
_g259 --
_g11.5
_tAge estimates
_g261 --
_g11.6
_tStar formation histories
_g264 --
_g12
_tDisk evolution and planet formation
_g268 --
_g12.1
_tClearing of optically thick disks
_g269 --
_g12.2
_tViscous disk evolution
_g272 --
_g12.3
_tBinaries
_g275 --
_g12.4
_tDisk evaporation
_g276 --
_g12.5
_tDust evolution
_g279 --
_g12.6
_tCore accretion and planet formation
_g284 --
_g12.7
_tGaseous gravitational instability and planet formation
_g285 --
_g12.8
_tMigration
_g286 --
_g12.9
_tDisk gaps and holes
_g287 --
_g12.10
_tDebris disks
_g288 --
_g12.11
_tSpeculations
_g290 --
_gAppendix 1
_tBasic hydrodynamic and MHD equations
_g292 --
_gAppendix 2
_tJeans masses and fragmentation
_g294 --
_gAppendix 3
_tBasic radiative transfer
_g298.
520 _aOur understanding of the formation of stars and planetary systems has changed greatly since the first edition of this book was published. This new edition has been thoroughly updated, and now includes material on molecular clouds, binaries, star clusters and the stellar initial mass function (IMF), disk evolution and planet formation. This book provides a comprehensive picture of the formation of stars and planetary systems, from their beginnings in cold clouds of molecular gas to their emergence as new suns with planet-forming disks. At each stage gravity induces an inward accretion of mass, and this is a central theme for the book. The author brings together current observations, rigorous treatments of the relevant astrophysics, and 150 illustrations, to clarify the sequence of events in star and planet formation. It is a comprehensive account of the underlying physical processes of accretion for graduate students and researchers.
650 0 _aStars
_xFormation.
650 0 _aAccretion (Astrophysics)
650 0 _aDisks (Astrophysics)
650 0 _aGravitational collapse.
776 0 8 _iPrint version:
_z9780521825016
830 0 _aCambridge astrophysics series ;
_v47.
856 4 0 _uhttps://doi.org/10.1017/CBO9780511552090
999 _c517737
_d517735