DISTANCE DETERMINATIONS TO SHIELD GALAXIES FROM HUBBLE SPACE TELESCOPE IMAGING
Here, we measure the distances to the 12 SHIELD galaxies to be between 5 and 12 Mpc by applying the tip of the red giant method to the resolved stellar populations imaged by the Hubble Space Telescope. Based on these distances, the HI masses in the sample range from 4x10 super(6) to 6x10 super(7) M...
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| Veröffentlicht in: | The Astrophysical journal 2014-04, Vol.785 (1), p.1-13 |
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| container_title | The Astrophysical journal |
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| creator | McQuinn, Kristen B W Cannon, John M Dolphin, Andrew E Skillman, Evan D Salzer, John J Haynes, Martha P Adams, Elizabeth Cave, Ian Elson, Ed C Giovanelli, Riccardo Ott, Juergen Saintonge, Amelie |
| description | Here, we measure the distances to the 12 SHIELD galaxies to be between 5 and 12 Mpc by applying the tip of the red giant method to the resolved stellar populations imaged by the Hubble Space Telescope. Based on these distances, the HI masses in the sample range from 4x10 super(6) to 6x10 super(7) M sub([middot in circle]), with a median HI mass of 1x10 super(7) M sub([middot in circle]). The tip of the red giant branch distances are up to 73% farther than flow-model estimates in the ALFALFA catalog. Five of the galaxies are part of the NGC 672 and NGC 784 groups, which together constitute a single structure. One galaxy is part of a larger linear ensemble of nine systems that stretches 1.6 Mpc from end to end. Three galaxies reside in regions with 1-9 neighbors, and four galaxies are truly isolated with no known system identified within a radius of 1 Mpc. |
| doi_str_mv | 10.1088/0004-637X/785/1/3 |
| format | Article |
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Based on these distances, the HI masses in the sample range from 4x10 super(6) to 6x10 super(7) M sub([middot in circle]), with a median HI mass of 1x10 super(7) M sub([middot in circle]). The tip of the red giant branch distances are up to 73% farther than flow-model estimates in the ALFALFA catalog. Five of the galaxies are part of the NGC 672 and NGC 784 groups, which together constitute a single structure. One galaxy is part of a larger linear ensemble of nine systems that stretches 1.6 Mpc from end to end. Three galaxies reside in regions with 1-9 neighbors, and four galaxies are truly isolated with no known system identified within a radius of 1 Mpc.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/785/1/3</identifier><language>eng</language><publisher>United States</publisher><subject>Alfalfa ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; CHARGES ; DISTANCE ; Estimates ; EVOLUTION ; FLOW MODELS ; GALAXIES ; Hubble Space Telescope ; Imaging ; LUMINOSITY ; MASS ; Red giant stars ; RED SHIFT ; Shields ; SPACE ; STARS ; Stellar populations ; TELESCOPES ; WAVELENGTHS</subject><ispartof>The Astrophysical journal, 2014-04, Vol.785 (1), p.1-13</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c339t-fa9cf418d35afabd4e5d81551eff9c3efc4855c1dd6cf677a4dc4f7b7ecac1e13</citedby><cites>FETCH-LOGICAL-c339t-fa9cf418d35afabd4e5d81551eff9c3efc4855c1dd6cf677a4dc4f7b7ecac1e13</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,27903,27904</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22357209$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>McQuinn, Kristen B W</creatorcontrib><creatorcontrib>Cannon, John M</creatorcontrib><creatorcontrib>Dolphin, Andrew E</creatorcontrib><creatorcontrib>Skillman, Evan D</creatorcontrib><creatorcontrib>Salzer, John J</creatorcontrib><creatorcontrib>Haynes, Martha P</creatorcontrib><creatorcontrib>Adams, Elizabeth</creatorcontrib><creatorcontrib>Cave, Ian</creatorcontrib><creatorcontrib>Elson, Ed C</creatorcontrib><creatorcontrib>Giovanelli, Riccardo</creatorcontrib><creatorcontrib>Ott, Juergen</creatorcontrib><creatorcontrib>Saintonge, Amelie</creatorcontrib><title>DISTANCE DETERMINATIONS TO SHIELD GALAXIES FROM HUBBLE SPACE TELESCOPE IMAGING</title><title>The Astrophysical journal</title><description>Here, we measure the distances to the 12 SHIELD galaxies to be between 5 and 12 Mpc by applying the tip of the red giant method to the resolved stellar populations imaged by the Hubble Space Telescope. Based on these distances, the HI masses in the sample range from 4x10 super(6) to 6x10 super(7) M sub([middot in circle]), with a median HI mass of 1x10 super(7) M sub([middot in circle]). The tip of the red giant branch distances are up to 73% farther than flow-model estimates in the ALFALFA catalog. Five of the galaxies are part of the NGC 672 and NGC 784 groups, which together constitute a single structure. One galaxy is part of a larger linear ensemble of nine systems that stretches 1.6 Mpc from end to end. Three galaxies reside in regions with 1-9 neighbors, and four galaxies are truly isolated with no known system identified within a radius of 1 Mpc.</description><subject>Alfalfa</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>CHARGES</subject><subject>DISTANCE</subject><subject>Estimates</subject><subject>EVOLUTION</subject><subject>FLOW MODELS</subject><subject>GALAXIES</subject><subject>Hubble Space Telescope</subject><subject>Imaging</subject><subject>LUMINOSITY</subject><subject>MASS</subject><subject>Red giant stars</subject><subject>RED SHIFT</subject><subject>Shields</subject><subject>SPACE</subject><subject>STARS</subject><subject>Stellar populations</subject><subject>TELESCOPES</subject><subject>WAVELENGTHS</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><recordid>eNqNkUFPg0AQhTdGE2v1B3gj8eIF2WFZFo603VISCk2hSW8buuxGTFuUpQf_vZAaz55eJu-bSeY9hJ4BvwEOAgdj7Nk-YXuHBdQBh9ygCVAS2B6h7BZN_vx79GDMxzi6YThB2SIpyiibc2vBS75dJ1lUJnlWWGVuFauEpwsrjtJon_DCWm7ztbXazWYpt4pNNOyUPOXFPN9wK1lHcZLFj-hOV0ejnn51inZLXs5XdprHyTxKbUlI2Nu6CqX2IKgJrXR1qD1F6wAoBaV1KInS0gsolVDXvtQ-Y5VXS0-zA1OykqCATNHL9W5r-kYY2fRKvsv2fFayF647_OzicKBer9Rn135dlOnFqTFSHY_VWbUXI4BBEPosdOEfKAaKPWBkQOGKyq41plNafHbNqeq-BWAxliHGdMUYthjKECAI-QFisXWa</recordid><startdate>20140410</startdate><enddate>20140410</enddate><creator>McQuinn, Kristen B W</creator><creator>Cannon, John M</creator><creator>Dolphin, Andrew E</creator><creator>Skillman, Evan D</creator><creator>Salzer, John J</creator><creator>Haynes, Martha P</creator><creator>Adams, Elizabeth</creator><creator>Cave, Ian</creator><creator>Elson, Ed C</creator><creator>Giovanelli, Riccardo</creator><creator>Ott, Juergen</creator><creator>Saintonge, Amelie</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20140410</creationdate><title>DISTANCE DETERMINATIONS TO SHIELD GALAXIES FROM HUBBLE SPACE TELESCOPE IMAGING</title><author>McQuinn, Kristen B W ; Cannon, John M ; Dolphin, Andrew E ; Skillman, Evan D ; Salzer, John J ; Haynes, Martha P ; Adams, Elizabeth ; Cave, Ian ; Elson, Ed C ; Giovanelli, Riccardo ; Ott, Juergen ; Saintonge, Amelie</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c339t-fa9cf418d35afabd4e5d81551eff9c3efc4855c1dd6cf677a4dc4f7b7ecac1e13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Alfalfa</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>CHARGES</topic><topic>DISTANCE</topic><topic>Estimates</topic><topic>EVOLUTION</topic><topic>FLOW MODELS</topic><topic>GALAXIES</topic><topic>Hubble Space Telescope</topic><topic>Imaging</topic><topic>LUMINOSITY</topic><topic>MASS</topic><topic>Red giant stars</topic><topic>RED SHIFT</topic><topic>Shields</topic><topic>SPACE</topic><topic>STARS</topic><topic>Stellar populations</topic><topic>TELESCOPES</topic><topic>WAVELENGTHS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>McQuinn, Kristen B W</creatorcontrib><creatorcontrib>Cannon, John M</creatorcontrib><creatorcontrib>Dolphin, Andrew E</creatorcontrib><creatorcontrib>Skillman, Evan D</creatorcontrib><creatorcontrib>Salzer, John J</creatorcontrib><creatorcontrib>Haynes, Martha P</creatorcontrib><creatorcontrib>Adams, Elizabeth</creatorcontrib><creatorcontrib>Cave, Ian</creatorcontrib><creatorcontrib>Elson, Ed C</creatorcontrib><creatorcontrib>Giovanelli, Riccardo</creatorcontrib><creatorcontrib>Ott, Juergen</creatorcontrib><creatorcontrib>Saintonge, Amelie</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>McQuinn, Kristen B W</au><au>Cannon, John M</au><au>Dolphin, Andrew E</au><au>Skillman, Evan D</au><au>Salzer, John J</au><au>Haynes, Martha P</au><au>Adams, Elizabeth</au><au>Cave, Ian</au><au>Elson, Ed C</au><au>Giovanelli, Riccardo</au><au>Ott, Juergen</au><au>Saintonge, Amelie</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>DISTANCE DETERMINATIONS TO SHIELD GALAXIES FROM HUBBLE SPACE TELESCOPE IMAGING</atitle><jtitle>The Astrophysical journal</jtitle><date>2014-04-10</date><risdate>2014</risdate><volume>785</volume><issue>1</issue><spage>1</spage><epage>13</epage><pages>1-13</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>Here, we measure the distances to the 12 SHIELD galaxies to be between 5 and 12 Mpc by applying the tip of the red giant method to the resolved stellar populations imaged by the Hubble Space Telescope. Based on these distances, the HI masses in the sample range from 4x10 super(6) to 6x10 super(7) M sub([middot in circle]), with a median HI mass of 1x10 super(7) M sub([middot in circle]). The tip of the red giant branch distances are up to 73% farther than flow-model estimates in the ALFALFA catalog. Five of the galaxies are part of the NGC 672 and NGC 784 groups, which together constitute a single structure. One galaxy is part of a larger linear ensemble of nine systems that stretches 1.6 Mpc from end to end. Three galaxies reside in regions with 1-9 neighbors, and four galaxies are truly isolated with no known system identified within a radius of 1 Mpc.</abstract><cop>United States</cop><doi>10.1088/0004-637X/785/1/3</doi><tpages>13</tpages></addata></record> |
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| subjects | Alfalfa ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CHARGES DISTANCE Estimates EVOLUTION FLOW MODELS GALAXIES Hubble Space Telescope Imaging LUMINOSITY MASS Red giant stars RED SHIFT Shields SPACE STARS Stellar populations TELESCOPES WAVELENGTHS |
| title | DISTANCE DETERMINATIONS TO SHIELD GALAXIES FROM HUBBLE SPACE TELESCOPE IMAGING |
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