000 04564nam a22004815i 4500
001 978-1-4020-6544-6
003 DE-He213
005 20161121231044.0
007 cr nn 008mamaa
008 100301s2008 ne | s |||| 0|eng d
020 _a9781402065446
_9978-1-4020-6544-6
024 7 _a10.1007/978-1-4020-6544-6
_2doi
050 4 _aQB4
072 7 _aPG
_2bicssc
072 7 _aSCI004000
_2bisacsh
072 7 _aNAT033000
_2bisacsh
082 0 4 _a520
_223
100 1 _aMilone, Eugene F.
_eauthor.
245 1 0 _aShort-Period Binary Stars: Observations, Analyses, and Results
_h[electronic resource] /
_cby Eugene F. Milone, Denis A. Leahy, David W. Hobill.
264 1 _aDordrecht :
_bSpringer Netherlands,
_c2008.
300 _aXVII, 270 p.
_bonline resource.
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
347 _atext file
_bPDF
_2rda
490 1 _aAstrophysics and Space Science Library,
_x0067-0057 ;
_v352
505 0 _aCompact Relativistic Binary Systems -- Black Hole Binaries: The Journey from Astrophysics to Physics -- Searches for Gravitational Waves from Binary Neutron Stars: A Review -- Observations of the Double Pulsar PSR J0737–3039A/B -- Gravitational Lensing in Compact Binary Systems -- Accreting Neutron Star Binaries -- Accreting Neutron Stars in Low-Mass X-Ray Binary Systems -- Observations and Modeling of Accretion Flows in X-ray Binaries -- Cataclysmic Variable Systems -- Modeling the Hot Components in Cataclysmic Variables: Info on the White Dwarf and Hot Disk from GALEX, FUSE, HST and SDSS -- The Cool Components in Cataclysmic Variables: Recent Advances and New Puzzles -- Models for Dynamically Stable Cataclysmic Variable Systems -- Modeling Short-Period Eclipsing Binaries -- Distance Estimation for Eclipsing X-ray Pulsars -- The Tools of the Trade and the Products they Produce: Modeling of Eclipsing Binary Observables -- The Closest of the Close: Observational and Modeling Progress -- Aspects of Short-Period Binary Evolution -- Common Envelope Evolution Redux.
520 _aShort-period binaries run the gamut from widely separated stars to black-hole pairs; in between are systems that include neutron stars and white dwarfs, and partially evolved systems such as tidally distorted and over-contact systems. These objects represent stages of evolution of binary stars, and their degrees of separation provide critical clues to how their evolutionary paths differ from that of single stars. The widest and least distorted systems provide astronomers with the essential precise data needed to study all stars: mass and radius. The interactions of binary star components, on the other hand, provide a natural laboratory to observe how the matter in these stars behaves under different and often varying physical conditions. Thus, cataclysmic variables with and without overpoweringly strong magnetic fields, and stars with densities from that found in the Sun to the degenerate matter of white dwarfs and the ultra-compact states of neutron stars and black holes are all discussed. The extensive index permits cross-referencing. The objects being discussed are carefully defined in each section and the contributions are organized according to the compactness of the binaries that are treated. Some treatments are of individual objects; others are more general. The observational techniques that are used by the contributors to throw light on these objects include gravitational wave investigations, X-ray, radio, infrared, and optical astronomy; and the ways in which these objects are analyzed is also discussed. Among the specific objects reported is the Double Pulsar, highlighting what observations of this object tell us about fundamental physics. The level of the book is appropriate for both professional astronomers in the field as well as people interested in other fields and dedicated amateur astronomers.
650 0 _aPhysics.
650 0 _aObservations, Astronomical.
650 0 _aAstronomy
_xObservations.
650 1 4 _aPhysics.
650 2 4 _aAstronomy, Observations and Techniques.
700 1 _aLeahy, Denis A.
_eauthor.
700 1 _aHobill, David W.
_eauthor.
710 2 _aSpringerLink (Online service)
773 0 _tSpringer eBooks
776 0 8 _iPrinted edition:
_z9781402065439
830 0 _aAstrophysics and Space Science Library,
_x0067-0057 ;
_v352
856 4 0 _uhttp://dx.doi.org/10.1007/978-1-4020-6544-6
912 _aZDB-2-PHA
950 _aPhysics and Astronomy (Springer-11651)
999 _c507885
_d507885