Absolute distance determination for objects of high redshift

Details Absolute distance determination for objects of high redshift Absolute distance determination for objects of high redshift

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983liaco..24..289s&link_type=abstract

IN: Quasars and gravitational lenses; Proceedings of the Twenty-fourth Liege International Astrophysical Colloguium, Cointe-Ougr

Astronomy and Astrophysics

Astrophysics

Astrometry, Extragalactic Radio Sources, Red Shift, Distance, Stimulated Emission

Scientific paper

Fundamental, redshift-independent methods of determining distances to extragalactic objects which by-pass the extragalactic distance ladder, and which are based on the intrinsic properties of the objects themselves, are discussed. A brief analytical exposition is given of a method of determining absolute distances from measurements of the emission, absorption, and angular size properties of objects. The specific application of this method in combination with the Sunyaev-Zeldovich effect and with stimulated radio recombination line emission to determine absolute distances is addressed.

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