Basit öğe kaydını göster

Enhanced x-ray emission coinciding with giant radio pulses from the Crab Pulsar

dc.contributor.authorRay, Paul S.
dc.contributor.authorGuver, Tolga
dc.contributor.authorHo, Wynn C. G.
dc.contributor.authorMalacaria, Christian
dc.contributor.authorMajid, Walid A.
dc.contributor.authorEnoto, Teruaki
dc.contributor.authorTerasawa, Toshio
dc.contributor.authorKisaka, Shota
dc.contributor.authorHu, Chin-Ping
dc.contributor.authorGuillot, Sebastien
dc.contributor.authorLewandowska, Natalia
dc.contributor.authorJaisawal, Gaurava K.
dc.contributor.authorFoster, Rick
dc.contributor.authorMurata, Yasuhiro
dc.contributor.authorTakeuchi, Hiroshi
dc.contributor.authorTakefuji, Kazuhiro
dc.contributor.authorSekido, Mamoru
dc.contributor.authorYonekura, Yoshinori
dc.contributor.authorMisawa, Hiroaki
dc.contributor.authorTsuchiya, Fuminori
dc.contributor.authorAoki, Takahiko
dc.contributor.authorTokumaru, Munetoshi
dc.contributor.authorHonma, Mareki
dc.contributor.authorKameya, Osamu
dc.contributor.authorOyama, Tomoaki
dc.contributor.authorAsano, Katsuaki
dc.contributor.authorShibata, Shinpei
dc.contributor.authorTanaka, Shuta J.
dc.contributor.authorBogdanov, Slavko
dc.contributor.authorKenyon, Steve
dc.contributor.authorSoong, Yang
dc.contributor.authorMarkwardt, Craig B.
dc.contributor.authorWadiasingh, Zorawar
dc.contributor.authorGendreau, Keith C.
dc.contributor.authorArzoumanian, Zaven
dc.contributor.authorOkajima, Takashi
dc.contributor.authorHarding, Alice K.
dc.date.accessioned2021-12-10T12:29:10Z
dc.date.available2021-12-10T12:29:10Z
dc.date.issued2021
dc.identifier.citationEnoto T., Terasawa T., Kisaka S., Hu C., Guillot S., Lewandowska N., Malacaria C., Ray P. S. , Ho W. C. G. , Harding A. K. , et al., "Enhanced x-ray emission coinciding with giant radio pulses from the Crab Pulsar", SCIENCE, cilt.372, sa.6538, ss.187-244, 2021
dc.identifier.issn0036-8075
dc.identifier.othervv_1032021
dc.identifier.otherav_bfc265e3-5b25-4e51-aba8-cb68ef08b9f0
dc.identifier.urihttp://hdl.handle.net/20.500.12627/173987
dc.identifier.urihttps://doi.org/10.1126/science.abd4659
dc.description.abstractGiant radio pulses (GRPs) are sporadic bursts emitted by some pulsars that last a few microseconds and are hundreds to thousands of times brighter than regular pulses from these sources. The only GRP-associated emission outside of radio wavelengths is from the Crab Pulsar, where optical emission is enhanced by a few percentage points during GRPs. We observed the Crab Pulsar simultaneously at x-ray and radio wavelengths, finding enhancement of the x-ray emission by 3.8 +/- 0.7% (a 5.4 sigma detection) coinciding with GRPs. This implies that the total emitted energy from GRPs is tens to hundreds of times higher than previously known. We discuss the implications for the pulsar emission mechanism and extragalactic fast radio bursts.
dc.language.isoeng
dc.subjectÇOK DİSİPLİNLİ BİLİMLER
dc.subjectMultidisciplinary
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectDoğa Bilimleri Genel
dc.titleEnhanced x-ray emission coinciding with giant radio pulses from the Crab Pulsar
dc.typeMakale
dc.relation.journalSCIENCE
dc.contributor.departmentRIKEN , ,
dc.identifier.volume372
dc.identifier.issue6538
dc.identifier.startpage187
dc.identifier.endpage244
dc.contributor.firstauthorID2639600


Bu öğenin dosyaları:

DosyalarBoyutBiçimGöster

Bu öğe ile ilişkili dosya yok.

Bu öğe aşağıdaki koleksiyon(lar)da görünmektedir.

Basit öğe kaydını göster