| Springer Verlag

134,540원  | 20160823  | 9783662500606

The basics of classical astronomy and stellar astrophysics needed for extragalactic astronomy are provided in the appendix.

 | Springer Nature B.V.

74,480원  | 20140312  | 9783662137147

This collection of papers presents a rather complete review of current knowledge of hot spots in some strong extragalactic radio sources. An overview of known results along with new data on radio observations and optical observations is given in the first and second parts of the book. Recent computational techniques which allow modelling and simulations of hot spots and jet behaviour are presented in the third part. The fourth part discusses particle acceleration and shock front phenomena.

De Young, David S.  | University of Chicago Press

129,060원  | 20020101  | 9780226144153

Extragalactic radio sources are among the most unusual and spectacular objects in the universe, with sizes in excess of millions of light years, radiated energies over ten times those of normal galaxies, and a unique morphology. They reveal some o...

 | Content Technologies, Inc.

0원  | 20130519  | 9781490200149

Never HIGHLIGHT a Book Again! Includes all testable terms, concepts, persons, places, and events.

 | Content Technologies, Inc.

0원  | 20120119  | 9781618120458

Never HIGHLIGHT a Book Again! Includes all testable terms, concepts, persons, places, and events. Cram101 Just the FACTS101 studyguides gives all of the outlines, highlights, and quizzes for your textbook with optional online comprehensive practice tests. Only Cram101 is Textbook Specific. Accompanies: 9783540331742. This item is printed on demand.

Schneider, Peter  | Springer

142,460원  | 20141124  | 9783642540820

The basics of classical astronomy and stellar astrophysics needed for extragalactic astronomy are provided in the appendix.

 | Springer

0원  | 20040101  | 9783540201281

Schneider, Peter  | Springer

0원  | 20060715  | 9783540331742

 | Scholars' Press

253,300원  | 20140614  | 9783639716634

Extragalactic sources of high-energy cosmic gamma-rays, like blazars and quasars, are usually highly variable and the temporal characteristics of their light curves are key to the understanding of their physics. In order to deal with blazar flares in different parts of electromagnetic spectrum - from gamma-rays and X-rays to visible light - we developed a new approach to correlation study based on Monte Carlo simulations and the Fourier convolution.

 | Kluwer Academic Publishers

184,380원  | 19980630  | 9780792350255

This book reproduces the proceedings of the last of a series of "Euroconferences" dedicated to the ongoing near-infrared sky surveys DENIS and 2MASS. It presents the current status and recent results of both projects. An analysis of the relevant results of the space mission MSX is also presented.

 | Dissertation Discovery Company, LLC

171,250원  | 20190531  | 9780530007137

Abstract:First documented staistical correlation between radio & optical events in variable extra-galactic sources.Dissertation Discovery Company and University of Florida are dedicated to making scholarly works more discoverable and accessible throughout the world. This dissertation, "Search for Correlated Radio and Optical Events in Long-term Studies of Extragalactic Sources" by Richard Bryan Pomphrey, was obtained from University of Florida and is being sold with permission from the author.

 | Dissertation Discovery Company

122,830원  | 20190531  | 9780530007120

Abstract:First documented staistical correlation between radio & optical events in variable extra-galactic sources.Dissertation Discovery Company and University of Florida are dedicated to making scholarly works more discoverable and accessible throughout the world. This dissertation, "Search for Correlated Radio and Optical Events in Long-term Studies of Extragalactic Sources" by Richard Bryan Pomphrey, was obtained from University of Florida and is being sold with permission from the author.

 | Dissertation.com

37,150원  | 20080701  | 9781599426846

According to astrophysical theory, magnetic fields should play an important role in the structure and dynamics of the interstellar medium. While astronomical observations confirm this directly, the observational record is sparse. This is because magnetic fields can only be measured via polarimetric methods, and most of these methods can only provide an indirect inference of the magnetic field strength.