ASCA Observation of Bright X-Ray Sources in the Nearby Spiral Galaxy IC 342

Okada Kyoko; Dotani Tadayasu; Makishima Kazuo; Mitsuda Kazuhisa; Mihara Tatehiro

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ASCA Observation of Bright X-Ray Sources in the Nearby Spiral Galaxy IC 342

机译：ASCA观测附近螺旋银河IC 342中的明亮X射线源

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X-rayobservationsofthenearbystarburstgalaxyIC342withASCAledtothedetectionofthreebrightX-raysources,whosepositionsareconsistentwiththosefromtheEinsteinandROSATobservations.TheX-rayluminositiesofthetwosourcesexceedtheEddingtonlimitofa1.4Ma??objectbytwoordersofmagnitudeforanassumeddistanceof4.5Mpc.Thebrightestone(source1)amongthethreeexhibitedsignificanttimevariationsonatimescaleofafewhoursduringtheASCAobservation.Thus,thesizeoftheemissionregionmustbesmallerthanabout1014cm.Theenergyspectrumofthesourcecanberepresentedeitherbyapower-lawwithanexponentialroll-over,orbyanopticallythickaccretiondiskmodelwithamaximumcolortemperatureof1.77keV.Althoughthelargeluminosityofsource1maybeexplainedbyaa??100Ma??blackholeat4.5Mpc,theobservedenergyspectrumistoohardtobeaccountedforbyanopticallythickaccretiondiskaroundtheblackhole.Ifsource1isarelativisticjetsourcewithstrongX-raybeaming,boththelargeluminosityandthehardX-rayspectrumcanbeexplained.

机译：X-rayobservationsofthenearbystarburstgalaxyIC342withASCAledtothedetectionofthreebrightX-raysources，whosepositionsareconsistentwiththosefromtheEinsteinandROSATobservations.TheX-rayluminositiesofthetwosourcesexceedtheEddingtonlimitofa1.4Ma ?? objectbytwoordersofmagnitudeforanassumeddistanceof4.5Mpc.Thebrightestone（source1中）amongthethreeexhibitedsignificanttimevariationsonatimescaleofafewhoursduringtheASCAobservation.Thus，thesizeoftheemissionregionmustbesmallerthanabout1014cm.Theenergyspectrumofthesourcecanberepresentedeitherbyapower-lawwithanexponentialroll过度，orbyanopticallythickaccretiondiskmodelwithamaximumcolortemperatureof1.77keV.Althoughthelargeluminosityofsource1maybeexplainedbyaa ?? 100MA ?? blackholeat4.5Mpc，theobservedenergyspectrumistoohardtobeaccountedforbyanopticallythickaccretiondiskaroundtheblackhole如果源1是具有强X射线光束的相对论性喷气机源，则可以解释大的发光度和硬X射线光谱。

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《PASJ: Publications of the Astronomical Society of Japan》 |1998年第1期|共页
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Okada Kyoko; Dotani Tadayasu; Makishima Kazuo; Mitsuda Kazuhisa; Mihara Tatehiro;
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1. ASCA Observation of Ultra-Luminous X-Ray Sources in the Nearby Spiral Galaxy NGC 2403 [J] . Kotoku Junichi, Mizuno Tsunefumi, Kubota Aya, PASJ: Publications of the Astronomical Society of Japan . 2000,第6期

机译：螺旋星系NGC 2403附近的超发光X射线源的ASCA观测
2. ASCA Observations of Two Ultra-Luminous Compact X-Ray Sources in the Edge-On Spiral Galaxy NGC 4565 [J] . Mizuno Tsunefumi, Ohnishi Tomohisa, Kubota Aya, PASJ: Publications of the Astronomical Society of Japan . 1999,第5期

机译：边缘螺旋银河NGC 4565中两个超发光紧凑型X射线源的ASCA观测
3. ACCRETION DISK SPECTRA OF ULTRALUMINOUS X-RAY SOURCES IN NEARBY SPIRAL GALAXIES AND GALACTIC SUPERLUMINAL JET SOURCES [J] . KEN EBISAWA, PIOTR ZYCKI, AYA KUBOTA, The Astrophysical journal . 2003,第2aaParta1期

机译：邻近螺旋星系和银河超发光射源中超X射线源的吸积谱
4. ULTRALUMINOUS X-RAY SOURCES IN NEARBY GALAXIES: CLUES ON THEIR NATURE FROM X-RAY TIMING AND NEW OPTICAL DATA [C] . L. Zampieri, P. Mucciarelli, R. Falomo, Conference on X-ray Universe . 2006

机译：附近星系的超易X射线源：来自X射线时序和新光学数据的本质上的线索
5. Multiwavelength analyses of a small sample of nearby spiral galaxies: The radio and X-ray connection. [D] . Maddox, Larry Allen. 2006

机译：对附近旋涡星系的一个小样本进行多波长分析：无线电和X射线连接。
6. JUNGFRAU detector for brighter x-ray sources: Solutions for IT and data science challenges in macromolecular crystallography [O] . Filip Leonarski, Aldo Mozzanica, Martin Brückner, 2020

机译：JUNGFRAU探测器用于更亮的X射线源：大分子晶体学中IT和数据科学挑战的解决方案
7. ASCA Observations of Two Ultra-Luminous Compact X-Ray Sources in the Edge-on Spiral Galaxy NGC 4565 [O] . Mizuno, Tsunefumi, Ohnishi, Tomohisa, Kubota, Aya, 1999

机译：asCa对两种超发光紧凑型X射线源的观察 Edge-on spiral Galaxy NGC 4565

ASCA Observation of Bright X-Ray Sources in the Nearby Spiral Galaxy IC 342

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