Spiral-like structure in the core of nearby galaxy clusters
Not surprisingly, with the very high angular resolution of the Chandra telescope, results revealed fairly complex structures in cluster cores to be more common than expected. In particular, understanding the nature of spiral-like features at the center of some clusters is the major motivation of thi...
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creator | Lagana, Tatiana F. Andrade-Santos, Felipe Lima Neto, Gastao B. |
description | Not surprisingly, with the very high angular resolution of the Chandra telescope, results revealed fairly complex structures in cluster cores to be more common than expected. In particular, understanding the nature of spiral-like features at the center of some clusters is the major motivation of this work. We present results from Chandra deep observations of 15 nearby galaxy clusters (0.01 |
doi_str_mv | 10.1063/1.3475240 |
format | Conference Proceeding |
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In particular, understanding the nature of spiral-like features at the center of some clusters is the major motivation of this work. We present results from Chandra deep observations of 15 nearby galaxy clusters (0.01<z<0.06). Using X-ray temperature and substructure maps, we detect a plume-like feature in the core of 7 clusters: A85, A426, A496, Hydra A, Centaurus, A1644 and Ophiuchus. 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In particular, understanding the nature of spiral-like features at the center of some clusters is the major motivation of this work. We present results from Chandra deep observations of 15 nearby galaxy clusters (0.01<z<0.06). Using X-ray temperature and substructure maps, we detect a plume-like feature in the core of 7 clusters: A85, A426, A496, Hydra A, Centaurus, A1644 and Ophiuchus. Comparing our results to numerical simulations, our investigation lends support to the fact that these patterns are due to nonzero impact parameter mergers.</description><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>BRIGHTNESS</subject><subject>COMPARATIVE EVALUATIONS</subject><subject>COMPUTERIZED SIMULATION</subject><subject>ELECTROMAGNETIC RADIATION</subject><subject>EVALUATION</subject><subject>GALAXY CLUSTERS</subject><subject>IMPACT PARAMETER</subject><subject>IONIZING RADIATIONS</subject><subject>OPTICAL PROPERTIES</subject><subject>PHYSICAL PROPERTIES</subject><subject>RADIATIONS</subject><subject>RESOLUTION</subject><subject>SIMULATION</subject><subject>TELESCOPES</subject><subject>X RADIATION</subject><issn>0094-243X</issn><issn>1551-7616</issn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2010</creationdate><recordtype>conference_proceeding</recordtype><recordid>eNotzM1KAzEUQOEgCtbqwjcIuE69N_-DKylahYILFdyVJHNjR4cZmWTAvr2Crs63OoxdIqwQrLrGldLOSA1HbIHGoHAW7TFbADRaSK3eTtlZKR8AsnHOL9jN81c3hV703SfxUqc51Xki3g287omn8ddj5gOFKR74e-jD94Gnfi6VpnLOTnLoC138d8le7-9e1g9i-7R5XN9uxYheVZGM9cZl0tI5lxGxxQBIyngTJXpN1isL0cVok7JtVOg9ZWwblzJIbdSSXf19x1K7XUldpbRP4zBQqjuJGsGgVj-IjUdg</recordid><startdate>20100101</startdate><enddate>20100101</enddate><creator>Lagana, Tatiana F.</creator><creator>Andrade-Santos, Felipe</creator><creator>Lima Neto, Gastao B.</creator><scope>OTOTI</scope></search><sort><creationdate>20100101</creationdate><title>Spiral-like structure in the core of nearby galaxy clusters</title><author>Lagana, Tatiana F. ; Andrade-Santos, Felipe ; Lima Neto, Gastao B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-o183t-c56857fe42777f111d1a01e3585b2184e68360b7bb6c36db3188ef1d97cf02453</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>2010</creationdate><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>BRIGHTNESS</topic><topic>COMPARATIVE EVALUATIONS</topic><topic>COMPUTERIZED SIMULATION</topic><topic>ELECTROMAGNETIC RADIATION</topic><topic>EVALUATION</topic><topic>GALAXY CLUSTERS</topic><topic>IMPACT PARAMETER</topic><topic>IONIZING RADIATIONS</topic><topic>OPTICAL PROPERTIES</topic><topic>PHYSICAL PROPERTIES</topic><topic>RADIATIONS</topic><topic>RESOLUTION</topic><topic>SIMULATION</topic><topic>TELESCOPES</topic><topic>X RADIATION</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Lagana, Tatiana F.</creatorcontrib><creatorcontrib>Andrade-Santos, Felipe</creatorcontrib><creatorcontrib>Lima Neto, Gastao B.</creatorcontrib><collection>OSTI.GOV</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Lagana, Tatiana F.</au><au>Andrade-Santos, Felipe</au><au>Lima Neto, Gastao B.</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Spiral-like structure in the core of nearby galaxy clusters</atitle><btitle>AIP conference proceedings</btitle><date>2010-01-01</date><risdate>2010</risdate><volume>1248</volume><issue>1</issue><issn>0094-243X</issn><eissn>1551-7616</eissn><abstract>Not surprisingly, with the very high angular resolution of the Chandra telescope, results revealed fairly complex structures in cluster cores to be more common than expected. In particular, understanding the nature of spiral-like features at the center of some clusters is the major motivation of this work. We present results from Chandra deep observations of 15 nearby galaxy clusters (0.01<z<0.06). Using X-ray temperature and substructure maps, we detect a plume-like feature in the core of 7 clusters: A85, A426, A496, Hydra A, Centaurus, A1644 and Ophiuchus. Comparing our results to numerical simulations, our investigation lends support to the fact that these patterns are due to nonzero impact parameter mergers.</abstract><cop>United States</cop><doi>10.1063/1.3475240</doi></addata></record> |
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subjects | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BRIGHTNESS COMPARATIVE EVALUATIONS COMPUTERIZED SIMULATION ELECTROMAGNETIC RADIATION EVALUATION GALAXY CLUSTERS IMPACT PARAMETER IONIZING RADIATIONS OPTICAL PROPERTIES PHYSICAL PROPERTIES RADIATIONS RESOLUTION SIMULATION TELESCOPES X RADIATION |
title | Spiral-like structure in the core of nearby galaxy clusters |
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