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1987•The Astrophysical Journal Supplement SeriesRequires access

The case low-dispersion northern sky survey. IV - Galaxies in the Bootes void region

N. Sanduleak, Peter Pesch

Open publisher page 27 citations

Abstract

Positions, estimated magnitudes, and finding charts (when needed) are provided for 424 blue and/or emission-line galaxies and 50 probable H II regions in 21 galaxies contained within the region 14h00m < R.A. < 15h30m and +33°.0 < decl. < +56°.0 (1950). These were identified on low-dispersion, objective-prism plates taken with the Burrell Schmidt-type telescope at Kitt Peak. This sample, which includes galaxies as faint as the 18th blue magnitude, should prove useful in further studies of the Bootes void.

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What this paper is about

Positions, estimated magnitudes, and finding charts (when needed) are provided for 424 blue and/or emission-line galaxies and 50 probable H II regions in 21 galaxies contained within the region 14h00m < R.A. < 15h30m and +33°.0 < decl. < +56°.0 (1950). These were identified on low-dispersion, objective-prism plates taken with the Burrell Schmidt-type telescope at Kitt Peak. This sample, which includes galaxies as faint as the 18th blue magnitude, should prove useful in further studies of the Bootes void.

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OpenAlex reports 27 citations for this work. Citation counts describe recorded attention and do not establish research quality.

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Available abstract

Positions, estimated magnitudes, and finding charts (when needed) are provided for 424 blue and/or emission-line galaxies and 50 probable H II regions in 21 galaxies contained within the region 14h00m < R.A. < 15h30m and +33°.0 < decl. < +56°.0 (1950). These were identified on low-dispersion, objective-prism plates taken with the Burrell Schmidt-type telescope at Kitt Peak. This sample, which includes galaxies as faint as the 18th blue magnitude, should prove useful in further studies of the Bootes void.

Key concepts: Sky, Void (composites), Astrophysics, Geology, Geography, Physics, Environmental science, Materials science

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