Very-High Energy Gamma-ray Astronomy: Search for Periodicity in Emission of Very High Energy Gamma-rays from the Supernova Remnant MSH 15-52
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Very-High Energy Gamma-ray Astronomy Search for Periodicity in Emission of Very High Energy Gamma-rays from the Supernova Remnant MSH 15-52
DE PB NWISBN: 9783639364620 bzw. 3639364627, in Deutsch, VDM Verlag Dr. Müller, Taschenbuch, neu.
Von Händler/Antiquariat, BuySomeBooks [52360437], Las Vegas, NV, U.S.A.
Paperback. 124 pages. Dimensions: 8.7in. x 5.9in. x 0.3in.In 2004, for the first time in the history of very-high energy gamma-ray astronomy, diffuse emission of gamma-rays from a pulsar wind nebula, was observed from the supernova remnant, MSH 15-52, by the H. E. S. S (High Energy Stereoscopic System). The supernova remnant (SNR), MSH 15-52, consisting of a PWN which is powered by a 150 millisecond relatively young and energetic pulsar, B1509-58, was observed with H. E. S. S. during 23 nights. The likelihood of the pulsar periodicity being propagated into the PWN emission was investigated, by searching for periodicity of VHE gamma-ray emission at and near the radio period from the entire composite supernova remnant. Fourier analysis techniques were employed for searching for a pulsed signal. This was done via the well-known universally most powerful (UMP) test, the Rayleigh test, and the H-test. No pulsed emission could be seen using the Rayleigh test and the H-test. The Eadie combination method of Rayleigh test results also showed no evidence of strong flares. Therefore, there was no compelling evidence of pulsed VHE gamma-ray emission from the supernova remnant MSH 15-52 at and near the known pulsar radio period. This item ships from multiple locations. Your book may arrive from Roseburg,OR, La Vergne,TN.
Paperback. 124 pages. Dimensions: 8.7in. x 5.9in. x 0.3in.In 2004, for the first time in the history of very-high energy gamma-ray astronomy, diffuse emission of gamma-rays from a pulsar wind nebula, was observed from the supernova remnant, MSH 15-52, by the H. E. S. S (High Energy Stereoscopic System). The supernova remnant (SNR), MSH 15-52, consisting of a PWN which is powered by a 150 millisecond relatively young and energetic pulsar, B1509-58, was observed with H. E. S. S. during 23 nights. The likelihood of the pulsar periodicity being propagated into the PWN emission was investigated, by searching for periodicity of VHE gamma-ray emission at and near the radio period from the entire composite supernova remnant. Fourier analysis techniques were employed for searching for a pulsed signal. This was done via the well-known universally most powerful (UMP) test, the Rayleigh test, and the H-test. No pulsed emission could be seen using the Rayleigh test and the H-test. The Eadie combination method of Rayleigh test results also showed no evidence of strong flares. Therefore, there was no compelling evidence of pulsed VHE gamma-ray emission from the supernova remnant MSH 15-52 at and near the known pulsar radio period. This item ships from multiple locations. Your book may arrive from Roseburg,OR, La Vergne,TN.
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Very-High Energy Gamma-ray Astronomy (2011)
DE PB NWISBN: 9783639364620 bzw. 3639364627, in Deutsch, VDM, Taschenbuch, neu.
Lieferung aus: Schweiz, Versandfertig innert 4 - 7 Werktagen.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
3
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Very-High Energy Gamma-Ray Astronomy (Paperback) (2011)
DE PB NW RPISBN: 9783639364620 bzw. 3639364627, in Deutsch, VDM Verlag, Germany, Taschenbuch, neu, Nachdruck.
Lieferung aus: Vereinigtes Königreich Großbritannien und Nordirland, Versandkostenfrei.
Von Händler/Antiquariat, The Book Depository EURO [60485773], London, United Kingdom.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
Von Händler/Antiquariat, The Book Depository EURO [60485773], London, United Kingdom.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
4
Very-High Energy Gamma-ray Astronomy
DE NWISBN: 9783639364620 bzw. 3639364627, in Deutsch, VDM Verlag Dr. Müller, Saarbrücken, Deutschland, neu.
Lieferung aus: Deutschland, zzgl. Versandkosten, Sofort lieferbar.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
5
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Very-High Energy Gamma-ray Astronomy (2011)
DE PB NW RPISBN: 9783639364620 bzw. 3639364627, in Deutsch, VDM Verlag Jul 2011, Taschenbuch, neu, Nachdruck.
Von Händler/Antiquariat, AHA-BUCH GmbH [51283250], Einbeck, Germany.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
6
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Very-High Energy Gamma-ray Astronomy: Search for Periodicity in Emission of Very High Energy Gamma-rays from the Supernova Remnant MSH 15-52
DE PB NWISBN: 9783639364620 bzw. 3639364627, in Deutsch, VDM Verlag Dr. Müller, Taschenbuch, neu.
Von Händler/Antiquariat, ExtremelyReliable [8304062], RICHMOND, TX, U.S.A.
This item is printed on demand.
This item is printed on demand.
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