Titlebook: Galaxy Distances and Deviations from Universal Expansion; Barry F. Madore,R. Breant Tully Book 1986 D. Reidel Publishing Company, Dordrech

PRE

A Solar Hydrogen Energy System,nearly complete sample of Sbc, Sc galaxies does not show any distance bias in the (Malmquist-free) log v. vs. M(B) relation. This demonstrates that even the latter relation can be applied only to well defined samples of type-restricted galaxies, if unbiased distances are aimed at.

overreach

abolish

Main Sequence Fitting and the Distance to the Large Magellanic Cloud,rs. The sources of random and systematic error are briefly discussed, and the effects due to convective overshoot are estimated. The possibility of extending this technique to other galaxies is mentioned.

前奏曲

圖表證明

Physical Models of Supernovae and the Distance Scale,to the use of supernovae as distance indicators. In particular, we wish to emphasize that theoretical supernova atmosphere calculations are now available to effect the connection between observations and hydrodynamical models.

Endearing

21cm Line Widths and Distances of Spiral Galaxies,nearly complete sample of Sbc, Sc galaxies does not show any distance bias in the (Malmquist-free) log v. vs. M(B) relation. This demonstrates that even the latter relation can be applied only to well defined samples of type-restricted galaxies, if unbiased distances are aimed at.

Brain-Waves

I Versus B-I Color-Magnitude Relation for Galaxies and I Band Distances,et al. 1979). The difference in the slopes of the blue and infrared Tully-Fisher relations implies that correlations must exist between color and 21-cm line width as well as color and absolute magnitude (Tully et al. 1982).

救護(hù)車

The Luminosity Index as a Distance Indicator and the Structure of the Virgo Cluster,and to confusion between the Virgo cluster proper (the S-cloud) and adjacent, but unrelated clouds at different distances. Two tests are presented which confirm the small scatter (σ ≈ 0.4 mag) of the corrected magnitude-luminosity index correlation (RC2 system) in the Virgo S cloud and in the Hercules supercluster.

Limpid

Infrared Colour-Luminosity Relations for Field Galaxies,o point for spirals can be reduced by incorporating a surface brightness correction. These developments suggest that colour-luminosity studies will continue to be a valuable check on velocities fields derived from the Tully-Fisher method.

易達(dá)到

Minimizing the Scatter in the Tully-Fisher Relation,urate to 1?%. The present scatter in the Tully-Fisher relation thus needs to be reduced by a factor of 2. In this contribution, we report on the sources of scatter in the Tully-Fisher relation and elaborate on a possible scheme which yields a scatter of only ?.25 mag.