Skip to product information
Frontiers of Space and Ground-Based Astronomy: The Astrophysics of the 21st Century (1994)

Frontiers Of Space And Ground-Based Astronomy

$329.99
Shipping calculated at checkout.
  • Authorized Dealer
  • Ships within 1 business day
  • Free 30-Day Returns
  • Secure Checkout via Shopify Payments
Details

"Frontiers Of Space And Ground-Based Astronomy" by Willem Wamsteker, Malcolm S. Longair, Y. Kondo is a astronomy book and space science reference focused on General Astronomy. Best for students, researchers, and serious astronomy enthusiasts.

ROSAT Observations G. HASINGER Max-Planck-Institut flir extraterrestrische Physik, D-85740 Garching, Germany Abstract. This review describes the most recent advances in the study of the extragalactic soft X-ray background and what we can learn about its constituents. The deepest pointed observations with the ROSAT PSPC are discussed. The logN-logS relation is presented, which reaches to the faintest X-ray fluxes and to the highest AGN surface densities ever achieved. The N(>S) relation shows a 2 density in excess of 400 deg- at the faintest fluxes and a flattening below the Einstein Deep Survey limit. About 60% of the extragalactic background has been resolved in the deepest field. Detailed source spectra and first optical and radio identifications will be discussed. The results are put into perspective of the higher energy X -ray background. Key words: X-rays, background radiations, active galactic nuclei. 1. Introduction The extragalactic X-ray background (XRB), discovered about 30 years ago, has been studied extensively with many X-ray experiments, in particular with the satel lites HEAO I and II (see ego Boldt 1987) and with ROSAT (e. g. Hasinger et aI. , 1993). Figure 1 shows a compilation of some of the most recent spectral measure ments for the X-ray background. Over the energy range from 3 to about 100 keY its spectrum can be well approximated by an optically thin thermal bremsstrahlung model with kT ~ 40 keY, while at lower X-ray energies a steepening into a new component has been observed observed (e. g.

Materials + Care

We prioritize quality in selecting the materials for our items, choosing premium fabrics and finishings that ensure durability, comfort, and timeless appeal.

Shipping + Returns

We strive to process and ship all orders in a timely manner, working diligently to ensure that your items are on their way to you as soon as possible.

Best For: Students and researchers interested in contemporary astrophysics and observational astronomy.
Focus: Recent advances in extragalactic soft X-ray background studies using ROSAT observations.
Covers: Analysis of ROSAT PSPC data, logN-logS relation, and the constituents of the soft X-ray background.
Why It Matters: Provides insight into the faintest X-ray sources and active galactic nuclei, contributing to understanding the structure and evolution of the universe.

"Frontiers Of Space And Ground-Based Astronomy" by Willem Wamsteker, Malcolm S. Longair, Y. Kondo is a astronomy book and space science reference focused on General Astronomy. Best for students, researchers, and serious astronomy enthusiasts.

Topic: General Astronomy

Author: Willem Wamsteker, Malcolm S. Longair, Y. Kondo

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

ROSAT Observations G. HASINGER Max-Planck-Institut flir extraterrestrische Physik, D-85740 Garching, Germany Abstract. This review describes the most recent advances in the study of the extragalactic soft X-ray background and what we can learn about its constituents. The deepest pointed observations with the ROSAT PSPC are discussed. The logN-logS relation is presented, which reaches to the faintest X-ray fluxes and to the highest AGN surface densities ever achieved. The N(>S) relation shows a 2 density in excess of 400 deg- at the faintest fluxes and a flattening below the Einstein Deep Survey limit. About 60% of the extragalactic background has been resolved in the deepest field. Detailed source spectra and first optical and radio identifications will be discussed. The results are put into perspective of the higher energy X -ray background. Key words: X-rays, background radiations, active galactic nuclei. 1. Introduction The extragalactic X-ray background (XRB), discovered about 30 years ago, has been studied extensively with many X-ray experiments, in particular with the satel lites HEAO I and II (see ego Boldt 1987) and with ROSAT (e. g. Hasinger et aI. , 1993). Figure 1 shows a compilation of some of the most recent spectral measure ments for the X-ray background. Over the energy range from 3 to about 100 keY its spectrum can be well approximated by an optically thin thermal bremsstrahlung model with kT ~ 40 keY, while at lower X-ray energies a steepening into a new component has been observed observed (e. g.

AuthorWillem Wamsteker, Malcolm S. Longair, Y. Kondo
PublisherSpringer Science & Business Media
Published1994-08-31
ISBN-139780792325277
BindingHardcover
Pages794
LanguageEnglish
SubjectsScience
TopicGeneral Astronomy
SeriesAstrophysics and Space Science Library

Format: Hardcover

Length: 794 pages

Language: English

Shop by collection

You might also like...