Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.atnf.csiro.au/pasa/15_1/valls-gabaud/paper/index.html
Äàòà èçìåíåíèÿ: Fri Apr 8 09:10:55 2016
Äàòà èíäåêñèðîâàíèÿ: Sun Apr 10 18:40:27 2016
Êîäèðîâêà:
Ïîèñêîâûå ñëîâà: ï ï ï ï ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï
Cosmological Applications of H Surveys

Cosmological Applications of Htex2html_wrap_inline452 Surveys

David Valls--Gabaud, PASA, 15 (1), 111
The html and gzipped postscript versions of this paper are in preprint form.
To access the final published version, download the pdf file.
Next Section: Diffuse H emission and
Contents Page: Volume 15, Number 1

Cosmological Applications of Htex2html_wrap_inline452 Surveys

David Valls-Gabaud tex2html_wrap_inline454

tex2html_wrap_inline456 UMR CNRS 7550, Observatoire de Strasbourg, 11 Rue de l'Universitö©, F-67000 Strasbourg
tex2html_wrap_inline458 Royal Greenwich Observatory, Madingley Road, Cambridge CB3 0EZ, UK
Email : dvg@astro.u-strasbg.fr dvg@ast.cam.ac.uk

Abstract:

We briefly review three main applications of Htex2html_wrap_inline452 surveys in cosmology, namely : (1) The diffuse Htex2html_wrap_inline452 emission as a tracer of the free-free foreground that contaminates the fluctuations in the cosmic microwave background radiation; (2) The Htex2html_wrap_inline452 emission from galaxies as a measure of the formation rate of massive stars, both at low and high redshift; (3) The diffuse Htex2html_wrap_inline452 emission from ionised clouds as a constraint on the local ionising background radiation.

Keywords: Cosmology : CMBR fluctuations, ionising background radiation - Galaxies : star formation rate


HTML SectionDownload Full Paper

Welcome... About Electronic PASA... Instructions to Authors
ASA Home Page... CSIRO Publishing PASA
Browse Articles HOME Search Articles
á© Copyright Astronomical Society of Australia 1997
ASKAP
Public