(Q59065711)

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The Hubble constant as derived from 21 cm linewidths

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The Hubble constant as derived from 21 cm linewidths (English)

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1

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Allan Sandage

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G. A. Tammann

2

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publication date

January 1984

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307

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5949

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326–329

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A distance scale from the infrared magnitude/H I velocity-width relation. IV. The morphological type dependence and scatter in the relation; the distances to nearby groups

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On the distance to M 33 determined from magnitude corrections to Hubble's original Cepheid photometry

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The distance to M 33 based on a new study of its Cepheids

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A composite period-luminosity relation for Cepheids at mean and maximum light

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The double Cepheid CE Cassiopeiae in NGC 7790: tests of the theory of the instability strip and the calibration of the period-luminosity-color relation

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The resolution of old red giant stars in the Sculptor group of galaxies

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A catalog of infrared magnitudes and HI velocity widths for nearby galaxies

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A distance scale from the infrared magnitude/H I velocity-width relation. II. The Virgo cluster

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A distance scale from the infrared magnitude/HI velocity-width relation. I. The calibration

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The infrared color-magnitude relation for early-type galaxies in Virgo and Coma

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Direct observations of the large-scale distribution of galaxies

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The Local Group: the solar motion relative to its centroid

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The Oosterhoff period groups and the age of globular clusters. III. The age of the globular cluster system

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Star clusters and stellar evolution. I. Improved synthetic color-magnitude diagrams for the oldest clusters

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The stellar content and distance of the galaxy NGC 2403 in the M 81 group

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Steps toward the Hubble constant. III. The distance and stellar content of the M 101 group of galaxies

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The brightest stars in nearby galaxies. II

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Redshift-distance relation. VII. Absolute magnitudes of the first ranked cluster galaxies as functions of cluster richness and Bautz-Morgan cluster type: the effect on qo

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10.1038/307326A0

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1984Natur.307..326S

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