THE COMA CLUSTER OF GALAXIES, I: SIZE AND STRUCTURE
Three independent counts of the Coma cluster of galaxies are intercompared. The three different surveys appear to be consistent with each other. It is concluded that this cluster contains some 800 members to photovisual magnitude about 18.5 and is about 100 minutes in radius. A possible spatial dens...
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creator | Omer,Guy C. ,Jr Page,Thornton L wilson,A. G |
description | Three independent counts of the Coma cluster of galaxies are intercompared. The three different surveys appear to be consistent with each other. It is concluded that this cluster contains some 800 members to photovisual magnitude about 18.5 and is about 100 minutes in radius. A possible spatial density distribution of the galaxies in this cluster is derived from the combined data. (Author)
Prepared for submission to the Astronomical Journal. Prepared in cooperation with California Univ., Los Angeles, and Wesleyan Univ., Middletown, Conn. |
format | Report |
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Prepared for submission to the Astronomical Journal. Prepared in cooperation with California Univ., Los Angeles, and Wesleyan Univ., Middletown, Conn.</description><subject>ASTRONOMY</subject><subject>COUNTING METHODS</subject><subject>DISTRIBUTION</subject><subject>GALAXIES</subject><subject>PHOTOGRAPHIC RECORDING SYSTEMS</subject><fulltext>true</fulltext><rsrctype>report</rsrctype><creationdate>1965</creationdate><recordtype>report</recordtype><sourceid>1RU</sourceid><recordid>eNrjZDAO8XBVcPb3dVRw9gkNDnENUvB3U3B39HGM8HQN1lHwtFII9oxyVXD0c1EIDgkKdQ4JDXLlYWBNS8wpTuWF0twMMm6uIc4euiklmcnxxSWZeakl8Y4uBmaGxmYmFsYEpAHrwiPA</recordid><startdate>196503</startdate><enddate>196503</enddate><creator>Omer,Guy C. ,Jr</creator><creator>Page,Thornton L</creator><creator>wilson,A. G</creator><scope>1RU</scope><scope>BHM</scope></search><sort><creationdate>196503</creationdate><title>THE COMA CLUSTER OF GALAXIES, I: SIZE AND STRUCTURE</title><author>Omer,Guy C. ,Jr ; Page,Thornton L ; wilson,A. G</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-dtic_stinet_AD06136483</frbrgroupid><rsrctype>reports</rsrctype><prefilter>reports</prefilter><language>eng</language><creationdate>1965</creationdate><topic>ASTRONOMY</topic><topic>COUNTING METHODS</topic><topic>DISTRIBUTION</topic><topic>GALAXIES</topic><topic>PHOTOGRAPHIC RECORDING SYSTEMS</topic><toplevel>online_resources</toplevel><creatorcontrib>Omer,Guy C. ,Jr</creatorcontrib><creatorcontrib>Page,Thornton L</creatorcontrib><creatorcontrib>wilson,A. G</creatorcontrib><creatorcontrib>RAND CORP SANTA MONICA CALIF</creatorcontrib><collection>DTIC Technical Reports</collection><collection>DTIC STINET</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Omer,Guy C. ,Jr</au><au>Page,Thornton L</au><au>wilson,A. G</au><aucorp>RAND CORP SANTA MONICA CALIF</aucorp><format>book</format><genre>unknown</genre><ristype>RPRT</ristype><btitle>THE COMA CLUSTER OF GALAXIES, I: SIZE AND STRUCTURE</btitle><date>1965-03</date><risdate>1965</risdate><abstract>Three independent counts of the Coma cluster of galaxies are intercompared. The three different surveys appear to be consistent with each other. It is concluded that this cluster contains some 800 members to photovisual magnitude about 18.5 and is about 100 minutes in radius. A possible spatial density distribution of the galaxies in this cluster is derived from the combined data. (Author)
Prepared for submission to the Astronomical Journal. Prepared in cooperation with California Univ., Los Angeles, and Wesleyan Univ., Middletown, Conn.</abstract><oa>free_for_read</oa></addata></record> |
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subjects | ASTRONOMY COUNTING METHODS DISTRIBUTION GALAXIES PHOTOGRAPHIC RECORDING SYSTEMS |
title | THE COMA CLUSTER OF GALAXIES, I: SIZE AND STRUCTURE |
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