Titlebook: Observational Cosmology; With the New Radio S M. N. Bremer,N. Jackson,I. Pérez-Fournon Conference proceedings 1998 Springer Science+Busines

Osmosis

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Flirtatious

The Cat: Cosmic Microwave Background Anisotropies and Sources at 15 GHzegree). This detection is consistent with a COBE-normalised CDM model, and provides constraints on the values of .. and Ω. The properties of discrete extragalactic radio sources at 15 GHz found in CAT fields are also discussed.

發(fā)電機

HST Imaging of 3CR Radio Galaxies: The Dust-Radio Connectiond the linear sizes of the dust features. The radio source has a preference to be perpendicular to the dust major axis when the dust is settled and localized (linear sizes < 2.5 kpc). There is no such a preference when the dust is distributed in a filamentary fashion throughout the radio galaxy.

Gnrh670

Current Status of Radio Source Databasesware tools to search and cross-identify radio sources from major catalogues. The latter evolved into “CATS” [6] maintained at Special Astrophysical Observatory (SAO, Russia), and is described in Section 2. The table collection of the first author is being folded into CATS.

Deduct

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Schlemms-Canal

Malcolm S. Longairod of vigorous policy activism has had an enduring legacy, nevertheless. No mainstream political party has seriously contemplated the reintroduction of racially discriminatory immigration policies. Cultural pluralism remains a lived reality and an organising principle of migrant settlement policies.