MARC Record from harvard_bibliographic_metadata

LEADER: 05427nam a22004695a 4500
001 014158917-5
005 20141003191018.0
008 130321s2003 ne | o ||0| 0|eng d
020 $a9789401707992
020 $a9789048162413 (ebk.)
020 $a9789401707992
020 $a9789048162413
024 7 $a10.1007/978-94-017-0799-2$2doi
035 $a(Springer)9789401707992
040 $aSpringer
050 4 $aQB460-466
072 7 $aPHVB$2bicssc
072 7 $aSCI005000$2bisacsh
082 04 $a523.01$223
100 1 $aThompson, Michael J.,$eeditor.
245 10 $aAsteroseismology Across the HR Diagram :$bProceedings of the Asteroseismology Workshop Porto, Portugal 1–5 July 2002 /$cedited by Michael J. Thompson, Margarida S. Cunha, Mário J. P. F. G. Monteiro.
246 3 $aProceedings of the Asteroseismology Workshop, held in Porto, Portugal, 1-5 July 2002
264 1 $aDordrecht :$bSpringer Netherlands :$bSpringer,$c2003.
300 $aXVIII, 294 p.$bonline resource.
336 $atext$btxt$2rdacontent
337 $acomputer$bc$2rdamedia
338 $aonline resource$bcr$2rdacarrier
347 $atext file$bPDF$2rda
505 0 $aSpace and Ground Based Data for Asteroseismology -- STARE Results on a Single Field: Tens of New Pulsating Stars -- The Eddington Mission -- Present Observational Status of Solar-Type Stars -- Present Observational Status of the Intermediate Mass Stars -- Present Observational Status of High Mass Pulsating Stars -- Old Pulsators: White Dwarfs and their Immediate Precursors -- ? Scuti Pulsations in Pre-Main Sequence Stars -- Solar-like Oscillations in Semiregular Variables -- Discovery of a New Class of Pulsating Stars: Gravity Mode Pulsators among Subdwarf B Stars -- Recent Observations of PMS ? Scuti Stars -- Multicolour Photometry for Mode Identification -- High-Resolution Spectroscopy for Mode Identification -- Theoretical Clues for Mode Identification — Instability Ranges and Rotational Splitting Patterns -- Peakbagging for Solar-Like Stars -- Mode Identification from Line Profiles Using the Direct Fitting Technique -- Statistical Revision of the Moment Method --
505 0 $aAn Improved Method of Photometric Mode Identification: Applications to Slowly Pulsating B, ? Cephei, ? Scuti and ? Doradus Stars -- Photometric Nonadiabatic Observables in Rotating ß Cephei Models -- Gravity Modes in Delta Scuti Stars -- Seismic Inference Using Genetic Algorithms -- Stellar Inversions -- On the Principal Asteroseismic Diagnostic Signatures -- Diagnostics of the Internal Structure of Stars Using the Differential Response Technique -- Stellar Convection -- Mixing and Diffusion in Stars -- Are Pulsation and Magnetic Axes Aligned in roAp Stars? -- Seismic Diagnostics of Stellar Convection Treatment from Oscillation Amplitudes of p-Modes -- Of Variability, or its Absence, in HgMn Stars -- A Study of the Solar-Like Properties of ? Hydri -- Giant Vibrations in Dip -- Stochastic Excitation of Gravity Waves by Overshooting Convection in Solar-Type Stars -- p-Mode Oscillations of ? Cen A -- Outstanding Issues for the Pulsation of Young Stars --
505 0 $aOutstanding Issues for Post-Main Sequence Evolution: Instability Strips and Excitation of Modes in Compact Pulsators -- Hot Subdwarfs: Magnetic, Oscillatory and other Physical Properties -- Nonlinearity of Nonradial Modes in Evolved Stars -- Summary: Problems, Connections and Expectations.
520 $aWe stand at the threshold of an exciting era of Asteroseismology. In a few months' time, the Canadian small-satellite asteroseismology mission MOST will be laun­ ched. Danish and French missions MONS and COROT should follow, with the ESA mission Eddington following in 2007/8. Helioseismology has proved spec­ tacularly successful in imaging the internal structure and dynamics of the Sun and probing the physics of the solar interior. Ground-based observations have detected solar-like oscillations on alpha Centauri A and other Sun-like stars, and diagnostics similar to those used in helioseismology are now being used to test and constrain the physics and evolutionary state of these stars. Multi-mode oscillations are being observed in an abundance of other stars, including slowly pulsating B stars (SPB stars), delta Scuti stars, Ap stars and the pulsating white dwarfs. New classes of pulsators continue to be discovered across the Hertzsprung-Russell diagram. For good reason it was decided to entitle our conference 'Asteroseismology Across the HR Diagram' . Yet the challenges still to be faced to make asteroseismology across the HR diagram a reality are formidable. Observation, data analysis and theory all pose hard problems to be overcome. In conceiving this meeting, the aim of the organisers was to facilitate a cross-fertilization of ideas and approaches between researchers working on different pulsators and with different areas of expertise. We venture to suggest that in this the conference was a great success.
650 10 $aPhysics.
650 0 $aPhysics.
650 24 $aAstronomy, Observations and Techniques.
650 24 $aAstrophysics and Astroparticles.
650 24 $aStatistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences.
700 1 $aMonteiro, Mário J. P. F. G.,$eeditor.
700 1 $aCunha, Margarida S.,$eeditor.
776 08 $iPrinted edition:$z9789048162413
988 $a20140910
906 $0VEN