The Status of the Distance Scale
arXiv:astro-ph/9911296
Abstract
Cepheids are the pillar of the extragalactic distance scale, but their reach in distance is not sufficient to calibrate H_0. Yet HST has provided Cepheid distances to eight galaxies which have produced SNe Ia. The latter are used as nearly perfect standard candles to carry the distance scale to 30,000 km/s, giving H_0 = 58 +/- 5. This determination finds support in other methods but its range in distance and its weight is unparalleled.
12 pages, 2 figures, 1 table, LaTeX 2.09. To appear in the Proceedings of the IAU Coll. 176 "The Impact of Large-Scale Surveys on Pulsating Star Research", Budapest, Aug. 1999, eds. L. Szabados & D. Kurtz (ASP Conf. Ser.)
References in corpus (13)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Explosion Models for Type Ia Supernovae: A Comparison with Observed Light Curves, distances, H_o and q_o
- BVRI Light Curves for 29 Type Ia Supernovae
- Type Ia Supernovae and the Hubble Constant
- A Local Hubble Bubble from SNe Ia?
- Cepheid Calibration of the Peak Brightness of SNe Ia -- IX. SN 1989B in NGC 3627
- Optical Light Curve of the Type Ia Supernova 1998bu in M96 and the Supernova Calibration of the Hubble Constant
- Determination of the Hubble constant from observations of Cepheid variables in the galaxy M96
- The evolution of ultraviolet emission lines from the circumstellar material surrounding SN 1987A
- The Virgo cluster distance from 21 cm-line widths
- On the Theoretical Period-Luminosity Relation of Cepheids
- Globular Cluster Calibration of the Peak Brightness of the Type Ia Supernova 1992A and the Value of Ho
- Cepheid models based on self-consistent stellar evolution and pulsation calculations: the right answer?