The Nuclei of Normal Galaxies

Andrew I. Harris

ISBN 10: 940104323X / ISBN 13: 9789401043236

Published by Springer Netherlands Nov 2012, 2012

About this Item

This item is printed on demand - it takes 3-4 days longer - Neuware -Our Galactic center's proximity allows astronomers to study physical pro cesses within galactic nuclei at a level of detail that will never be possible in the more distant, but usually also more spectacular, extragalactic systems. Recent advances in instrumentation from the radio, through the submillime ter and infrared wavebands, and out to the X- and ''(-ray bands now allow observations of the Galactic Center over thirteen orders of magnitude in wave length. Our knowledge about the central few hundred parsecs of our Galaxy has consequently increased vastly over the past decade. The same new instru ments provide high resolution, high quality measurements of nearby ''normal'' galactic nuclei; that is, nuclei whose modest energy output is comparable to that of our own (and most other) galaxies. Theorists, spurred in part by the new observations, have been able to refine models of the energetics, dynam ics, and evolution of the gas and stellar systems deep within galactic nuclei. 528 pp. Englisch.

Seller Inventory # 9789401043236

Bibliographic Details

• Title: The Nuclei of Normal Galaxies
• Publisher: Springer Netherlands Nov 2012
• Publication Date: 2012
• Language: English
• ISBN 10: 940104323X
• ISBN 13: 9789401043236
• Binding: Taschenbuch
• Condition: Neu
• Dimensions: 240W x 160H x 29D millimeters 240 millimeters width by 160 millimeters height by 29 millimeters depth
• Weight: 834 grams

About this title

Synopsis

Our Galactic center's proximity allows astronomers to study physical pro­ cesses within galactic nuclei at a level of detail that will never be possible in the more distant, but usually also more spectacular, extragalactic systems. Recent advances in instrumentation from the radio, through the submillime­ ter and infrared wavebands, and out to the X- and "'(-ray bands now allow observations of the Galactic Center over thirteen orders of magnitude in wave­ length. Our knowledge about the central few hundred parsecs of our Galaxy has consequently increased vastly over the past decade. The same new instru­ ments provide high resolution, high quality measurements of nearby ''normal'' galactic nuclei; that is, nuclei whose modest energy output is comparable to that of our own (and most other) galaxies. Theorists, spurred in part by the new observations, have been able to refine models of the energetics, dynam­ ics, and evolution of the gas and stellar systems deep within galactic nuclei.