Star formation with future millimetre and radio interferometers

Download
  1. Get@NRC: Star formation with future millimetre and radio interferometers (Opens in a new window)
DOIResolve DOI: http://doi.org/10.1017/S0074180900241909
AuthorSearch for:
TypeArticle
Proceedings titleStar Formation at High Angular Resolution
Series titleProceedings of the International Astronomical Union; Volume 221
ConferenceXXV General Assembly of the IAU, July 22-25, 2003, Sydney, Australia
ISSN1743-9213
1743-9221
Pages461470
AbstractThe Low Frequency Array (LOFAR), the Atacama Large Millimetre Array (ALMA), and the Square Kilometre Array (SKA) will be the largest and most capable aperture synthesis facilities of the next few decades. The advances in our knowledge of star formation that ALMA will permit are well known to the star formation community, but the potential of the SKA has so far attracted less attention. I will outline the star formation science cases of these upcoming facilities, with an emphasis on the SKA.
Publication date
PublisherCambridge University Press
International Astronomical Union
LanguageEnglish
AffiliationNational Research Council Canada; NRC Herzberg Institute of Astrophysics
Peer reviewedYes
NPARC number9723455
Export citationExport as RIS
Report a correctionReport a correction
Record identifieraed65df8-9eda-4356-bd3f-b232e1a3419c
Record created2009-07-17
Record modified2017-06-02
Bookmark and share
  • Share this page with Facebook (Opens in a new window)
  • Share this page with Twitter (Opens in a new window)
  • Share this page with Google+ (Opens in a new window)
  • Share this page with Delicious (Opens in a new window)