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Solar-Type Activity in Main-Sequence Stars (Astronomy and Astrophysics Library)
 
 
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Solar-Type Activity in Main-Sequence Stars (Astronomy and Astrophysics Library) [Hardcover]

Roald E. Gershberg (Author), Svetlana Knyazeva (Translator)

Price: $159.00 & this item ships for FREE with Super Saver Shipping. Details
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Book Description

August 22, 2005 3540212442 978-3540212447 1
The first comprehensive monograph on this active and productive field of research investigates solar-type activity amongst the large spectrum of low- and middle-mass main sequence stars, and presents the subject in a systematic and comprehensive fashion.

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From the Back Cover

Solar-type activity over the whole range of the electromagnetic spectrum is a phenomenon inherent in the majority of low- and moderate-mass main sequence stars. In this monograph observational results are summarized in a systematic and comprehensive fashion. The analysis of the various manifestations of such stellar activity leads to the identification of these phenomena with macroscopic non-linear processes in a magnetized plasma. Comparative study of flare stars and the Sun has become increasingly fruitful and is presently an active field of research involving stellar and solar physicists, experts in plasma physics and high-energy astrophysicists. This book will provide them with both an introduction and overview of observational results from the first optical photometry and spectroscopy, from the satellite telescopes International Ultraviolet Explorer to Hubble Space Telescope, XMM-Newton and Chandra, as well as with the present physical interpretation of solar-type activity in main sequence stars. Gershberg's 40-year career studying UV Cet type stars and related objects enables him to provide readers with expert insight into the characteristics of such stars in both the quiescent state and during flares and the reliability of the data over the electromagnetic spectrum and wide temporal scales.

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Inside This Book (learn more)
First Sentence:
In 1924, Hertzsprung noticed that one of the faint stars in Carina was brighter by 2m on one of the photographs taken on the night of January 29. Read the first page
Key Phrases - Statistically Improbable Phrases (SIPs): (learn more)
quiescent photosphere, known flare stars, active red dwarfs, stronger flare, strongest solar flares, calcium emission, cumulative energy spectrum, recorded flares, quiet radiation, flare continuum, red asymmetry, flare red dwarfs, quasistatic cooling, stellar flares, preflare brightening, photoelectric monitoring, solar content, supporting heating, flare decay, most active stars, active dwarfs, flare luminosity, surface filling factor, optical flares, chromospheric models
Key Phrases - Capitalized Phrases (CAPs): (learn more)
Einstein Observatory, Proxima Cen, Jodrell Bank, Prox Cen, Monsignori Fossi, Mount Wilson Observatory, General Description of Stellar Flares, Kitt Peak, Flares Table, Very Large Antenna, Analysis of Experiment, Star Date Experiment Strengthening Other, Stephanion Observatory, European Southern Observatory, Garcia López, Green Bank, New Mexico, South African Astronomical Observatory, Southern Africa, Special Astrophysical Observatory
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