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Quasar Parallax: a Method for Determining Direct Geometrical Distances to Quasars | | Martin Elvis
; Margarita Karovska
; | | Date: |
17 Nov 2002 | | Journal: | Astrophys.J. 581 (2002) L67-L70 | | Subject: | astro-ph | | Affiliation: | Harvard-Smithsonian Center for Astrophysics | | Abstract: | We describe a novel method to determine direct geometrical distances to quasars that can measure the cosmological constant, Lambda, with minimal assumptions. This method is equivalent to geometric parallax, with the `standard length’ being the size of the quasar broad emission line region (BELR) as determined from the light travel time measurements of reverberation mapping. The effect of non-zero Lambda on angular diameter is large, 40% at z=2, so mapping angular diameter distances vs. redshift will give Lambda with (relative) ease. In principle these measurements could be made in the UV, optical, near infrared or even X-ray bands. Interferometers with a resolution of 0.01mas are needed to measure the size of the BELR in z=2 quasars, which appear plausible given reasonable short term extrapolations of current technology. | | Source: | arXiv, astro-ph/0211385 | | Services: | Forum | Review | PDF | Favorites | |
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