THE BLACK HOLE MASS FUNCTION DERIVED FROM LOCAL SPIRAL GALAXIES
We present our determination of the nuclear supermassive black hole (SMBH) mass function for spiral galaxies in the local universe, established from a volume-limited sample consisting of a statistically complete collection of the brightest spiral galaxies in the southern ([delta] < 0]degrees]) he...
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| Veröffentlicht in: | The Astrophysical journal 2014-07, Vol.789 (2), p.1-16 |
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| container_title | The Astrophysical journal |
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| creator | Davis, Benjamin L Berrier, Joel C Johns, Lucas Shields, Douglas W Hartley, Matthew T Kennefick, Daniel Kennefick, Julia SEIGAR, MARC S Lacy, Claud H S |
| description | We present our determination of the nuclear supermassive black hole (SMBH) mass function for spiral galaxies in the local universe, established from a volume-limited sample consisting of a statistically complete collection of the brightest spiral galaxies in the southern ([delta] < 0]degrees]) hemisphere. The sample is defined by a limiting luminosity (redshift-independent) distance, D sub(L) = 25.4 Mpc (z = 0.00572) and a limiting absolute B-band magnitude, M sub(B) = -19.12. We then use an established relationship between the logarithmic spiral arm pitch angle and the mass of the central SMBH in a host galaxy in order to estimate the mass of the 128 respective SMBHs in this volume-limited sample. This result effectively gives us the distribution of mass for SMBHs residing in spiral galaxies over a lookback time, t sub(L) [< or =, slant] 82.1 h super(-1) sub(67.77) Myr and contained within a comoving volume, V sub(C) = 3.37 x 10 super(4) h super(-3) sub(67.77) M sub([middot in circle]) Mpc super(-3). |
| doi_str_mv | 10.1088/0004-637X/789/2/124 |
| format | Article |
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This result effectively gives us the distribution of mass for SMBHs residing in spiral galaxies over a lookback time, t sub(L) [< or =, slant] 82.1 h super(-1) sub(67.77) Myr and contained within a comoving volume, V sub(C) = 3.37 x 10 super(4) h super(-3) sub(67.77) M sub([middot in circle]) Mpc super(-3).</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/789/2/124</identifier><language>eng</language><publisher>United States</publisher><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; BARYONS ; BLACK HOLES ; Black holes (astronomy) ; Constraining ; COSMOLOGY ; DENSITY ; DISTRIBUTION ; DISTRIBUTION FUNCTIONS ; EVOLUTION ; GALAXIES ; Hemispheres ; LUMINOSITY ; MASS ; Pitch angle ; RED SHIFT ; Samples ; SIMULATION ; SPECTRA ; Spiral galaxies ; Statistical analysis ; Statistical methods ; UNIVERSE</subject><ispartof>The Astrophysical journal, 2014-07, Vol.789 (2), p.1-16</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c454t-acb49ff886b468b2e35997a3f57d75ac9aa4fe54902aa0ef62b6bc7f58d8a5eb3</citedby><cites>FETCH-LOGICAL-c454t-acb49ff886b468b2e35997a3f57d75ac9aa4fe54902aa0ef62b6bc7f58d8a5eb3</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/22365702$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Davis, Benjamin L</creatorcontrib><creatorcontrib>Berrier, Joel C</creatorcontrib><creatorcontrib>Johns, Lucas</creatorcontrib><creatorcontrib>Shields, Douglas W</creatorcontrib><creatorcontrib>Hartley, Matthew T</creatorcontrib><creatorcontrib>Kennefick, Daniel</creatorcontrib><creatorcontrib>Kennefick, Julia</creatorcontrib><creatorcontrib>SEIGAR, MARC S</creatorcontrib><creatorcontrib>Lacy, Claud H S</creatorcontrib><title>THE BLACK HOLE MASS FUNCTION DERIVED FROM LOCAL SPIRAL GALAXIES</title><title>The Astrophysical journal</title><description>We present our determination of the nuclear supermassive black hole (SMBH) mass function for spiral galaxies in the local universe, established from a volume-limited sample consisting of a statistically complete collection of the brightest spiral galaxies in the southern ([delta] < 0]degrees]) hemisphere. The sample is defined by a limiting luminosity (redshift-independent) distance, D sub(L) = 25.4 Mpc (z = 0.00572) and a limiting absolute B-band magnitude, M sub(B) = -19.12. We then use an established relationship between the logarithmic spiral arm pitch angle and the mass of the central SMBH in a host galaxy in order to estimate the mass of the 128 respective SMBHs in this volume-limited sample. This result effectively gives us the distribution of mass for SMBHs residing in spiral galaxies over a lookback time, t sub(L) [< or =, slant] 82.1 h super(-1) sub(67.77) Myr and contained within a comoving volume, V sub(C) = 3.37 x 10 super(4) h super(-3) sub(67.77) M sub([middot in circle]) Mpc super(-3).</description><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>BARYONS</subject><subject>BLACK HOLES</subject><subject>Black holes (astronomy)</subject><subject>Constraining</subject><subject>COSMOLOGY</subject><subject>DENSITY</subject><subject>DISTRIBUTION</subject><subject>DISTRIBUTION FUNCTIONS</subject><subject>EVOLUTION</subject><subject>GALAXIES</subject><subject>Hemispheres</subject><subject>LUMINOSITY</subject><subject>MASS</subject><subject>Pitch angle</subject><subject>RED SHIFT</subject><subject>Samples</subject><subject>SIMULATION</subject><subject>SPECTRA</subject><subject>Spiral galaxies</subject><subject>Statistical analysis</subject><subject>Statistical methods</subject><subject>UNIVERSE</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><recordid>eNqN0E9PwjAYx_HGaCKir8DLEi9e5rr-WduTmTBgcTDDwHBrutLGGWC4joPv3i0Yz56ePMknv8MXgPsQPoWQ8wBCSPwIs03AuAhQECJyAQYhxdwnmLJLMPgT1-DGuc_-RUIMwPNqlngvWTx69WZ5lnjzuCi8yXoxWqX5whsny_Q9GXuTZT73snwUZ17xli67M42zeJMmxS24smrnzN3vHYL1JFmNZn6WT9PO-5pQ0vpKl0RYy3lUkoiXyGAqBFPYUrZlVGmhFLGGEgGRUtDYCJVRqZmlfMsVNSUegofzbu3aSjpdtUZ_6PpwMLqVCOGIMog69XhWx6b-OhnXyn3ltNnt1MHUJydDFnIRRZiSf1AoQkYp71fxmeqmdq4xVh6baq-abxlC2feXfU7Z15Vdf4lk1x__AHgTcTc</recordid><startdate>20140710</startdate><enddate>20140710</enddate><creator>Davis, Benjamin L</creator><creator>Berrier, Joel C</creator><creator>Johns, Lucas</creator><creator>Shields, Douglas W</creator><creator>Hartley, Matthew T</creator><creator>Kennefick, Daniel</creator><creator>Kennefick, Julia</creator><creator>SEIGAR, MARC S</creator><creator>Lacy, Claud H S</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>20140710</creationdate><title>THE BLACK HOLE MASS FUNCTION DERIVED FROM LOCAL SPIRAL GALAXIES</title><author>Davis, Benjamin L ; Berrier, Joel C ; Johns, Lucas ; Shields, Douglas W ; Hartley, Matthew T ; Kennefick, Daniel ; Kennefick, Julia ; SEIGAR, MARC S ; Lacy, Claud H S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c454t-acb49ff886b468b2e35997a3f57d75ac9aa4fe54902aa0ef62b6bc7f58d8a5eb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>BARYONS</topic><topic>BLACK HOLES</topic><topic>Black holes (astronomy)</topic><topic>Constraining</topic><topic>COSMOLOGY</topic><topic>DENSITY</topic><topic>DISTRIBUTION</topic><topic>DISTRIBUTION FUNCTIONS</topic><topic>EVOLUTION</topic><topic>GALAXIES</topic><topic>Hemispheres</topic><topic>LUMINOSITY</topic><topic>MASS</topic><topic>Pitch angle</topic><topic>RED SHIFT</topic><topic>Samples</topic><topic>SIMULATION</topic><topic>SPECTRA</topic><topic>Spiral galaxies</topic><topic>Statistical analysis</topic><topic>Statistical methods</topic><topic>UNIVERSE</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Davis, Benjamin L</creatorcontrib><creatorcontrib>Berrier, Joel C</creatorcontrib><creatorcontrib>Johns, Lucas</creatorcontrib><creatorcontrib>Shields, Douglas W</creatorcontrib><creatorcontrib>Hartley, Matthew T</creatorcontrib><creatorcontrib>Kennefick, Daniel</creatorcontrib><creatorcontrib>Kennefick, Julia</creatorcontrib><creatorcontrib>SEIGAR, MARC S</creatorcontrib><creatorcontrib>Lacy, Claud H S</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>Davis, Benjamin L</au><au>Berrier, Joel C</au><au>Johns, Lucas</au><au>Shields, Douglas W</au><au>Hartley, Matthew T</au><au>Kennefick, Daniel</au><au>Kennefick, Julia</au><au>SEIGAR, MARC S</au><au>Lacy, Claud H S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>THE BLACK HOLE MASS FUNCTION DERIVED FROM LOCAL SPIRAL GALAXIES</atitle><jtitle>The Astrophysical journal</jtitle><date>2014-07-10</date><risdate>2014</risdate><volume>789</volume><issue>2</issue><spage>1</spage><epage>16</epage><pages>1-16</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>We present our determination of the nuclear supermassive black hole (SMBH) mass function for spiral galaxies in the local universe, established from a volume-limited sample consisting of a statistically complete collection of the brightest spiral galaxies in the southern ([delta] < 0]degrees]) hemisphere. The sample is defined by a limiting luminosity (redshift-independent) distance, D sub(L) = 25.4 Mpc (z = 0.00572) and a limiting absolute B-band magnitude, M sub(B) = -19.12. We then use an established relationship between the logarithmic spiral arm pitch angle and the mass of the central SMBH in a host galaxy in order to estimate the mass of the 128 respective SMBHs in this volume-limited sample. This result effectively gives us the distribution of mass for SMBHs residing in spiral galaxies over a lookback time, t sub(L) [< or =, slant] 82.1 h super(-1) sub(67.77) Myr and contained within a comoving volume, V sub(C) = 3.37 x 10 super(4) h super(-3) sub(67.77) M sub([middot in circle]) Mpc super(-3).</abstract><cop>United States</cop><doi>10.1088/0004-637X/789/2/124</doi><tpages>16</tpages><oa>free_for_read</oa></addata></record> |
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| source | IOP Publishing Free Content; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection |
| subjects | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BARYONS BLACK HOLES Black holes (astronomy) Constraining COSMOLOGY DENSITY DISTRIBUTION DISTRIBUTION FUNCTIONS EVOLUTION GALAXIES Hemispheres LUMINOSITY MASS Pitch angle RED SHIFT Samples SIMULATION SPECTRA Spiral galaxies Statistical analysis Statistical methods UNIVERSE |
| title | THE BLACK HOLE MASS FUNCTION DERIVED FROM LOCAL SPIRAL GALAXIES |
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