RE J1255+266—Detection of an Extremely Bright EUV Transient
During a pointed ROSAT observation in the direction of the Coma cluster of galaxies an exceptionally bright EUV source, RE J1255+266, was detected serendipitously. The source is located close to the Galactic North pole, at b II ~ 89°. Its observed EUV flux (62-110 eV) at the time of the detection wa...
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crcambridgeupr:10.1017/s025292110003640x 2024-03-03T08:47:15+00:00 RE J1255+266—Detection of an Extremely Bright EUV Transient Dahlem, Michael 1996 http://dx.doi.org/10.1017/s025292110003640x https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S025292110003640X en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms International Astronomical Union Colloquium volume 152, page 471-474 ISSN 0252-9211 journal-article 1996 crcambridgeupr https://doi.org/10.1017/s025292110003640x 2024-02-08T08:42:50Z During a pointed ROSAT observation in the direction of the Coma cluster of galaxies an exceptionally bright EUV source, RE J1255+266, was detected serendipitously. The source is located close to the Galactic North pole, at b II ~ 89°. Its observed EUV flux (62-110 eV) at the time of the detection was of order 7 × 10 −9 ergs s −1 cm −2 , making RE J1255+266 temporarily one of the brightest EUV sources on the sky. The EUV flare of RE J1255+266 has a light curve with a decay time of about 0.86 days. With respect to earlier non-detections, the source brightened by a factor of > 7000. Such a behavior has not been observed before. Thus, it is unclear what type of source RE J1255+266 might be. The most likely optical counterpart is a faint ( V ~ 18.5 mag) object with a blue spectrum (taken from an objective-prism Schmidt plate). For more details on the optical identification see the paper by J. Pye (this conference). Simultaneous observations with CGRO/BATSE resulted in non-detections of the source in the 8-50 keV energy range. Article in Journal/Newspaper North Pole Cambridge University Press North Pole International Astronomical Union Colloquium 152 471 474 |
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Cambridge University Press |
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English |
description |
During a pointed ROSAT observation in the direction of the Coma cluster of galaxies an exceptionally bright EUV source, RE J1255+266, was detected serendipitously. The source is located close to the Galactic North pole, at b II ~ 89°. Its observed EUV flux (62-110 eV) at the time of the detection was of order 7 × 10 −9 ergs s −1 cm −2 , making RE J1255+266 temporarily one of the brightest EUV sources on the sky. The EUV flare of RE J1255+266 has a light curve with a decay time of about 0.86 days. With respect to earlier non-detections, the source brightened by a factor of > 7000. Such a behavior has not been observed before. Thus, it is unclear what type of source RE J1255+266 might be. The most likely optical counterpart is a faint ( V ~ 18.5 mag) object with a blue spectrum (taken from an objective-prism Schmidt plate). For more details on the optical identification see the paper by J. Pye (this conference). Simultaneous observations with CGRO/BATSE resulted in non-detections of the source in the 8-50 keV energy range. |
format |
Article in Journal/Newspaper |
author |
Dahlem, Michael |
spellingShingle |
Dahlem, Michael RE J1255+266—Detection of an Extremely Bright EUV Transient |
author_facet |
Dahlem, Michael |
author_sort |
Dahlem, Michael |
title |
RE J1255+266—Detection of an Extremely Bright EUV Transient |
title_short |
RE J1255+266—Detection of an Extremely Bright EUV Transient |
title_full |
RE J1255+266—Detection of an Extremely Bright EUV Transient |
title_fullStr |
RE J1255+266—Detection of an Extremely Bright EUV Transient |
title_full_unstemmed |
RE J1255+266—Detection of an Extremely Bright EUV Transient |
title_sort |
re j1255+266—detection of an extremely bright euv transient |
publisher |
Cambridge University Press (CUP) |
publishDate |
1996 |
url |
http://dx.doi.org/10.1017/s025292110003640x https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S025292110003640X |
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North Pole |
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North Pole |
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North Pole |
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North Pole |
op_source |
International Astronomical Union Colloquium volume 152, page 471-474 ISSN 0252-9211 |
op_rights |
https://www.cambridge.org/core/terms |
op_doi |
https://doi.org/10.1017/s025292110003640x |
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International Astronomical Union Colloquium |
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152 |
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471 |
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474 |
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