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  • Cosmic Explosions in Three Dimensions

    inbunden, 2004, Engelska, ISBN 9780521842860
    Från 2043 kr

    Supernovae and gamma-ray bursts are the strongest explosions in the Universe. Observations show that, rather than being symmetrical, they are driven by strong jets of energy and

  • Cosmochemistry

    pocket, 2011, Engelska, ISBN 9780521169592
    Från 558 kr

    The chemical composition of the Universe has evolved over billions of years. A host of astrophysical processes and observations must be understood in order to explain why celestial

  • Type Ia Supernovae

    inbunden, 2000, Engelska, ISBN 9780521780360

    Observations of distant supernovae have recently provided startling evidence that the expansion of the Universe may be accelerating, rather than decelerating. If this result is

  • Structure Formation in Astrophysics

    pocket, 2011, Engelska, ISBN 9780521182744
    Från 553 kr

    Understanding the formation of objects at all scales in the universe, from galaxy clusters to stars and planets, is a major problem in modern astrophysics, and one of the most

  • X-ray Polarimetry

    inbunden, 2010, Engelska, ISBN 9780521191845

    Due to the advent of a new generation of detectors, X-ray polarimetry promises to join X-ray imaging, spectroscopy and timing as one of the main observational techniques in high

  • AGN Feedback in Galaxy Formation

    inbunden, 2010, Engelska, ISBN 9780521192545

    During the past decade, convincing evidence has been accumulated concerning the effect of active galactic nuclei (AGN) activity on the internal and external environment of their

  • Stellar Astrophysics for the Local Group

    inbunden, 1998, Engelska, ISBN 9780521632553

    With the advent of large, ground-based telescopes and space telescopes, it is now possible to study in detail stars outside our galaxy - in neighbouring galaxies in the so-called

  • The Metal-Rich Universe

    inbunden, 2008, Engelska, ISBN 9780521879989
    Från 2111 kr

    Metal-rich stars accumulate their metals from previous generations of stars, and so contain the history of their galaxy. By studying these stars we can gain valuable insights into