Skip to main content

Radio Astronomy and Cosmology

  • Book
  • © 1977

Overview

Part of the book series: International Astronomical Union Symposia (IAUS, volume 74)

This is a preview of subscription content, log in via an institution to check access.

Access this book

eBook USD 39.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 54.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access

Licence this eBook for your library

Institutional subscriptions

Table of contents (40 chapters)

  1. Surveys of Radio Sources, Source Counts and Anisotropies

  2. Spectral Index Distributions

  3. Angular Diameter-Redshift and Flux Density Tests

Keywords

About this book

337 F(e) = (z) where the angle between the directions III and 112 is equal to 8. r is the angular diameter effective distance of the epoch for recombination. F (8) ~ve have F(e) : f (e) ~ (S" ) e. . ~ is a Bessel function. It is assumed here that the spectrum of gravitational waves takes the form 1\ hI'::: hoK for all relevant wavelengths, a is beam width of the radio antenna, d\= d~, and ~ is the duration of the process of recombinations in \-time. The results for different beam widths are shown in Fig. 1. 338 I. D. NOVIKOV 1-. . . -__ 0. 5 1 1. 5 2 e' 0. 5 o and for a l' (solid line) and Fig. 1. The function f(8) for n for a = 2' (dotted line). These formula should be used in analysing the implications of future observations. Comparison with the observational data now available enables us to establish an upper limit for the energy density of long gravitational waves. This method is most sensitive for gravitational waves with A ~ ct The fluctuations ~; due to these waves have scale ~ 0. 03 GW rec 4 radian. If, according to modern observations, we take ~; < 10- , then 8 26 ~GW/Ey < 10- for those gravitational waves which have A = 5. 10 cm GW today where Ey is the energy density of relict radiation. The fluctuations ~TT due to long gravitational waves with A = ct .

Editors and Affiliations

  • Division of Radiophysics, CSIRO, Epping, Australia

    David L. Jauncey

Bibliographic Information

  • Book Title: Radio Astronomy and Cosmology

  • Editors: David L. Jauncey

  • Series Title: International Astronomical Union Symposia

  • DOI: https://doi.org/10.1007/978-94-010-1260-7

  • Publisher: Springer Dordrecht

  • eBook Packages: Springer Book Archive

  • Copyright Information: International Astronomical Union 1977

  • Softcover ISBN: 978-90-277-0839-7Published: 30 September 1977

  • eBook ISBN: 978-94-010-1260-7Published: 06 December 2012

  • Series ISSN: 1743-9213

  • Series E-ISSN: 2352-2186

  • Edition Number: 1

  • Number of Pages: 416

  • Number of Illustrations: 6 b/w illustrations

  • Topics: Classical and Quantum Gravitation, Relativity Theory

Publish with us