| Property |
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| dbo:abstract
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- Als Dark Flow (Dunkler Fluss) wird ein mögliches Muster in der Eigenbewegung von Galaxienhaufen bezeichnet. (de)
- Als Dark Flow (Dunkler Fluss) wird ein mögliches Muster in der Eigenbewegung von Galaxienhaufen bezeichnet. (de)
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| dbo:originalTitle
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- A measurement of large-scale peculiar velocities of clusters of galaxies: technical details (de)
- The Error Budget of the Dark Flow Measurement (de)
- A New Measurement of the Bulk Flow of X-Ray Luminous Clusters of Galaxies (de)
- A measurement of large-scale peculiar velocities of clusters of galaxies: results and cosmological implications. (de)
- Measuring the cosmological bulk flow using the peculiar velocities of supernovae (de)
- Measuring bulk motion of X-ray clusters via the kinematic Sunyaev-Zeldovich effect: summarizing the ”dark flow” evidence and its implications (de)
- A measurement of large-scale peculiar velocities of clusters of galaxies: technical details (de)
- The Error Budget of the Dark Flow Measurement (de)
- A New Measurement of the Bulk Flow of X-Ray Luminous Clusters of Galaxies (de)
- A measurement of large-scale peculiar velocities of clusters of galaxies: results and cosmological implications. (de)
- Measuring the cosmological bulk flow using the peculiar velocities of supernovae (de)
- Measuring bulk motion of X-ray clusters via the kinematic Sunyaev-Zeldovich effect: summarizing the ”dark flow” evidence and its implications (de)
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| prop-de:arxiv
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- 11020800 (xsd:integer)
- 12020717 (xsd:integer)
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| prop-de:autor
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- A. Kashlinsky, F. Atrio-Barandela, H. Ebeling
- Alexander Kashlinsky
- De-Chang Dai,W. H. Kinney, D. Stojkovic
- A. Kashlinsky, F. Atrio-Barandela, H. Ebeling, A. Edge, and D. Kocevski
- F. Atrio-Barandela, A. Kashlinsky, H. Ebeling, D. Kocevski, A. Edge
- A. Kashlinsky, F. Atrio-Barandela, D. Kocevski, H. Ebeling
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| prop-de:band
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- 686 (xsd:integer)
- 691 (xsd:integer)
- 712 (xsd:integer)
- 719 (xsd:integer)
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| prop-de:doi
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- 101086 (xsd:integer)
- 101088 (xsd:integer)
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| prop-de:jahr
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- 2008 (xsd:integer)
- 2009 (xsd:integer)
- 2010 (xsd:integer)
- 2011 (xsd:integer)
- 2012 (xsd:integer)
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| prop-de:monat
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- April
- August
- Februar
- Oktober
- Feb.
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| prop-de:nummer
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- 1 (xsd:integer)
- 2 (xsd:integer)
- 4 (xsd:integer)
- 77 (xsd:integer)
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| prop-de:online
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| prop-de:sammelwerk
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| prop-de:text
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- We detect motion along this axis, but right now our data cannot state as strongly as we'd like whether the clusters are coming or going
- At this point we don't have enough information to see what it is, or to constrain it. We can only say with certainty that somewhere very far away the world is very different than what we see locally. Whether it's 'another universe' or a different fabric of space-time we don't know.
- Because the dark flow already extends so far, it likely extends across the visible universe
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| prop-de:zugriff
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- 2012-04-27 (xsd:date)
- 2012-04-29 (xsd:date)
- 2012-11-19 (xsd:date)
- 2013-01-04 (xsd:date)
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| dct:subject
| |
| bibo:pages
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- 172
- 77–87
- 1479–1493
- L49–L52
- L81–L85
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| rdf:type
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| rdfs:comment
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- Als Dark Flow (Dunkler Fluss) wird ein mögliches Muster in der Eigenbewegung von Galaxienhaufen bezeichnet. (de)
- Als Dark Flow (Dunkler Fluss) wird ein mögliches Muster in der Eigenbewegung von Galaxienhaufen bezeichnet. (de)
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| rdfs:label
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- Dunkler Fluss (de)
- Dunkler Fluss (de)
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