A new γ-ray burst classification scheme from GRB 060614
Norris, J. P. ; Barthelmy, S. D. ; Granot, J. ; Kaneko, Y. ; Kouveliotou, C. ; Markwardt, C. B. ; Mészáros, P. ; Nakar, E. ; Nousek, J. A. ; O'Brien, P. T. ; Page, M. ; Palmer, D. M. ; Parsons, A. M. ; Roming, P. W. A. ; Sakamoto, T. ; Sarazin, C. L. ; Schady, P. ; Stamatikos, M. ; Woosley, S. E. ; Gehrels, N.
[s.l.] : Nature Publishing Group
Published 2006
[s.l.] : Nature Publishing Group
Published 2006
| ISSN: |
1476-4687
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| Source: |
Nature Archives 1869 - 2009
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| Topics: |
Biology
Chemistry and Pharmacology
Medicine
Natural Sciences in General
Physics
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| Notes: |
[Auszug] Gamma-ray bursts (GRBs) are known to come in two duration classes, separated at ∼2 s. Long-duration bursts originate from star-forming regions in galaxies, have accompanying supernovae when these are near enough to observe and are probably caused by massive-star collapsars. Recent ...
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| Type of Medium: |
Electronic Resource
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| URL: |
| _version_ | 1798293018982219777 |
|---|---|
| autor | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. |
| autorsonst | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. |
| book_url | http://dx.doi.org/10.1038/nature05376 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLZ234693886 |
| insertion_date | 1911-02-25 |
| issn | 1476-4687 |
| journal_name | Nature |
| materialart | 1 |
| notes | [Auszug] Gamma-ray bursts (GRBs) are known to come in two duration classes, separated at ∼2 s. Long-duration bursts originate from star-forming regions in galaxies, have accompanying supernovae when these are near enough to observe and are probably caused by massive-star collapsars. Recent ... |
| package_name | Nature Publishing Group |
| publikationsjahr_anzeige | 2006 |
| publikationsjahr_facette | 2006 |
| publikationsjahr_intervall | 7994:2005-2009 |
| publikationsjahr_sort | 2006 |
| publikationsort | [s.l.] |
| publisher | Nature Publishing Group |
| reference | 444 (2006), S. 1044-1046 |
| search_space | articles |
| shingle_author_1 | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. |
| shingle_author_2 | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. |
| shingle_author_3 | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. |
| shingle_author_4 | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. |
| shingle_catch_all_1 | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. A new γ-ray burst classification scheme from GRB 060614 Nature Publishing Group [Auszug] Gamma-ray bursts (GRBs) are known to come in two duration classes, separated at ∼2 s. Long-duration bursts originate from star-forming regions in galaxies, have accompanying supernovae when these are near enough to observe and are probably caused by massive-star collapsars. Recent ... 1476-4687 14764687 |
| shingle_catch_all_2 | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. A new γ-ray burst classification scheme from GRB 060614 Nature Publishing Group [Auszug] Gamma-ray bursts (GRBs) are known to come in two duration classes, separated at ∼2 s. Long-duration bursts originate from star-forming regions in galaxies, have accompanying supernovae when these are near enough to observe and are probably caused by massive-star collapsars. Recent ... 1476-4687 14764687 |
| shingle_catch_all_3 | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. A new γ-ray burst classification scheme from GRB 060614 Nature Publishing Group [Auszug] Gamma-ray bursts (GRBs) are known to come in two duration classes, separated at ∼2 s. Long-duration bursts originate from star-forming regions in galaxies, have accompanying supernovae when these are near enough to observe and are probably caused by massive-star collapsars. Recent ... 1476-4687 14764687 |
| shingle_catch_all_4 | Norris, J. P. Barthelmy, S. D. Granot, J. Kaneko, Y. Kouveliotou, C. Markwardt, C. B. Mészáros, P. Nakar, E. Nousek, J. A. O'Brien, P. T. Page, M. Palmer, D. M. Parsons, A. M. Roming, P. W. A. Sakamoto, T. Sarazin, C. L. Schady, P. Stamatikos, M. Woosley, S. E. Gehrels, N. A new γ-ray burst classification scheme from GRB 060614 Nature Publishing Group [Auszug] Gamma-ray bursts (GRBs) are known to come in two duration classes, separated at ∼2 s. Long-duration bursts originate from star-forming regions in galaxies, have accompanying supernovae when these are near enough to observe and are probably caused by massive-star collapsars. Recent ... 1476-4687 14764687 |
| shingle_title_1 | A new γ-ray burst classification scheme from GRB 060614 |
| shingle_title_2 | A new γ-ray burst classification scheme from GRB 060614 |
| shingle_title_3 | A new γ-ray burst classification scheme from GRB 060614 |
| shingle_title_4 | A new γ-ray burst classification scheme from GRB 060614 |
| sigel_instance_filter | dkfz geomar wilbert ipn albert |
| source_archive | Nature Archives 1869 - 2009 |
| timestamp | 2024-05-06T08:57:45.317Z |
| titel | A new γ-ray burst classification scheme from GRB 060614 |
| titel_suche | A new γ-ray burst classification scheme from GRB 060614 |
| topic | W V WW-YZ TA-TD U |
| uid | nat_lic_papers_NLZ234693886 |