Intrinsic Redshifts and the Tully–Fisher Distance Scale

Author: Russell, David

Source: Astrophysics and Space Science, Volume 299, Number 4, October 2005 , pp. 405-418(14)

Publisher: Springer

Buy & download fulltext article:

OR

Price: $47.00 plus tax (Refund Policy)

Abstract:

The Tully–Fisher relationship (TFR) has been shown to have a relatively small observed scatter of sim±0.35 mag implying an intrinsic scatter < ±0.30 mag. However, when the TFR is calibrated from distances derived from the Hubble relation for field galaxies scatter is consistently found to be ±0.64 to ±0.84 mag. This significantly larger scatter requires that intrinsic TFR scatter is actually much larger than ±0.30 mag, that field galaxies have an intrinsic TFR scatter much larger than cluster spirals, or that field galaxies have a velocity dispersion relative to the Hubble flow in excess of 1000 km s-1. Each of these potential explanations faces difficulties and contradicted by available data and the results of previous studies. An alternative explanation is that the measured redshifts of galaxies are composed of a cosmological redshift component predicted from the value of the Hubble constant and a superimposed intrinsic redshift component previously identified in other studies. This intrinsic redshift component may exceed 5000 km s-1 in individual galaxies. In this alternative scenario a possible value for the Hubble constant is 55–60 km s-1 Mpc-1.

Keywords: galaxies; distances and redshifts

Document Type: Research article

DOI: http://dx.doi.org/10.1007/s10509-005-3426-2

Affiliations: 1: Owego Free Academy, Owego, NY, USA, Email: russeld1@oagw.stier.org

Publication date: 2005-10-01

Related content

Key

Free Content
Free content
New Content
New content
Open Access Content
Open access content
Subscribed Content
Subscribed content
Free Trial Content
Free trial content

Text size:

A | A | A | A
Share this item with others: These icons link to social bookmarking sites where readers can share and discover new web pages. print icon Print this page