標題: Titlebook: Galactic Astrophysics and Gamma-Ray Astronomy; Proceedings of a Mee G. E. Morfill,R. Buccheri Conference proceedings 1983 D. Reidel Publish [打印本頁] 作者: Monomania 時間: 2025-3-21 17:54
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy影響因子(影響力)
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy影響因子(影響力)學科排名
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy網(wǎng)絡(luò)公開度
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy網(wǎng)絡(luò)公開度學科排名
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy被引頻次
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy被引頻次學科排名
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy年度引用
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy年度引用學科排名
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy讀者反饋
書目名稱Galactic Astrophysics and Gamma-Ray Astronomy讀者反饋學科排名
作者: insurrection 時間: 2025-3-21 23:44
Kathy Lee-Son,Massimo Attanasio in Patras, August 19, 1982. Roughly one hundred scientists attended this meeting, the discussions were lively — sometimes heated — and the original time span allocated to the meeting was a result, comfortably exceeded by about 50%.作者: inhibit 時間: 2025-3-22 01:25 作者: GROUP 時間: 2025-3-22 07:09 作者: Highbrow 時間: 2025-3-22 12:42
https://doi.org/10.1007/978-1-4613-4024-9ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hump is discussed.作者: periodontitis 時間: 2025-3-22 14:42 作者: periodontitis 時間: 2025-3-22 17:19
Cosmic Gamma Rays and Molecular Gas in the Galaxy,It is shown that, locally, γ-ray data enable the calibration of H. densities to be inferred from CO data and elsewhere the variation of cosmic-ray intensity with position to be assessed. Finally, the importance of cosmic-ray irradiated molecular clouds in simulating γ-ray ‘sources’ is reiterated.作者: 織物 時間: 2025-3-22 23:31 作者: 山頂可休息 時間: 2025-3-23 02:42
Comparison of Far-Infrared Radiation with Gamma Radiation,ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hump is discussed.作者: accomplishment 時間: 2025-3-23 09:26 作者: OVER 時間: 2025-3-23 14:03 作者: Tinea-Capitis 時間: 2025-3-23 19:05 作者: Interlocking 時間: 2025-3-23 22:26 作者: Nonconformist 時間: 2025-3-24 04:07 作者: 不確定 時間: 2025-3-24 07:08 作者: 除草劑 時間: 2025-3-24 13:26 作者: nonchalance 時間: 2025-3-24 17:41 作者: Boycott 時間: 2025-3-24 21:58 作者: PRE 時間: 2025-3-25 02:47
Randomized Encryption Techniquesns can initiate electro-optical showers, which provide a secondary particle population at a lower energy. Both gamma and radio radiation are thought to be explicable within this framework..We show that — because of the properties of curvature radiation — there is an intrinsic lower limit to the gamm作者: ACE-inhibitor 時間: 2025-3-25 05:55 作者: 認為 時間: 2025-3-25 07:52 作者: 有機體 時間: 2025-3-25 11:45 作者: 消音器 時間: 2025-3-25 19:00 作者: 織物 時間: 2025-3-25 21:05
Ali E. Karakaya,Semra Sardas,Sema Burgazces discovered by the COS-B satellite..32 low latitude (|.| < 5°) IPC fields, mosaic-arranged to cover the few-square-degrees COS-B error circles, yielded 30 soft X-ray sources, the fluxes of which range from ~ 1/100 to few UFU, and no diffuse features..While the density of ~ 1 source/IPC field is c作者: Seminar 時間: 2025-3-26 02:28
Using , for Two-Phase Flow in Porous Media COS-B. The consistency of the two datasets is discussed; while a satisfying general agreement is observed, a few distinct discrepancies point to possible time variations within the compact source component of the total galactic emission. The bulk of emission appears very well correlated to the colu作者: 袖章 時間: 2025-3-26 05:38
Background for Advances in Data Base Theoryal measurements are now available at those energies, where the contribution from π°-decay gamma rays can be neglected. The high MeV-fluxes observed in both parts of the Galaxy are an indication of either a strong electron induced component or a high contribution from unresolved sources. Several inte作者: somnambulism 時間: 2025-3-26 08:42
Eliminating Cycles in Database Schemas from galaxy counts. It is found that to a good approximation the gamma-ray intensity is proportional to the total gas column density, and on this basis a map of the angular distribution of local molecular hydrogen at intermediate latitudes is presented. Comparing this with a simular map produced fr作者: ACTIN 時間: 2025-3-26 15:31 作者: 并置 時間: 2025-3-26 19:28
https://doi.org/10.1007/978-1-4613-4024-9ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hum作者: 開花期女 時間: 2025-3-27 00:49 作者: Aids209 時間: 2025-3-27 04:26 作者: 混合,攙雜 時間: 2025-3-27 06:45 作者: 過去分詞 時間: 2025-3-27 10:00
Gamma Rays from Close Binary Systems,little interest for explaining the γ-ray sources discovered by the COS-B satellite. Accretion models where there is a non thermal component in the particle energy distribution may be relevant to γ-ray astronomy.作者: 斷言 時間: 2025-3-27 15:37 作者: 支形吊燈 時間: 2025-3-27 19:55
A Search for Counterparts of Selected Cos-B Galactic Gamma-Ray Sources: The X-Ray Survey and Opticang targets for the HRI instrument capable of an accuracy of ~ 3 arc sec..Due to the misfortunes which occurred to the Einstein satellite, this time-consuming process was feasible only in two cases: within the error circle of 2CG 135 + 01, the radio variable star LSI61.303 was pinpointed by the HRI, 作者: 浸軟 時間: 2025-3-28 00:30
Large-Scale Structure of the Galaxy and High-Energy Gamma-Ray Observations,d the gas is indicated by the gamma-ray data. The systematic variation with longitude of the spectrum of the gamma-ray emission points to an increased flux of cosmic-ray electrons in the 100 MeV to 1 GeV energy range in regions where dense clouds are concentrated. The variation could as well be due 作者: 不來 時間: 2025-3-28 04:47 作者: 剝削 時間: 2025-3-28 09:53
peration for another 5 to 10 years, and therefore it is hoped that the proceeding of this meeting can be used (in the intermediate time) as a basis for further studies, as a stimulation for more theoretical work and as an important contribution for defining the aims and operation of future gamma-ray missions.978-94-009-7210-0978-94-009-7208-7作者: cleaver 時間: 2025-3-28 10:33 作者: alliance 時間: 2025-3-28 15:47
Jürgen H. P. Hoffmeyer-Zlotnik,Christof Wolfnt of neutrino flux, combined with the measurement (or upper limit) of gamma-ray flux would show whether the active galactic nuclei are powered by massive black holes or spinars. We estimate that gamma rays would be degraded at spinars, too, at energies > 1 GeV.作者: CLAN 時間: 2025-3-28 20:22
Crowdsourcing in Higher Education,rces contains 25 sources, of which 21 are not yet unambiguously identified. Their average properties are discussed. The error region of the unidentified source 2CG195 + 04 (Geminga) is studied at other wavelengths in greatest detail. This search for a counterpart is summarized, showing the possibili作者: 階層 時間: 2025-3-29 02:50 作者: craving 時間: 2025-3-29 05:00 作者: CT-angiography 時間: 2025-3-29 09:14 作者: 甜食 時間: 2025-3-29 13:10 作者: 瑣事 時間: 2025-3-29 19:35
Preface, in Patras, August 19, 1982. Roughly one hundred scientists attended this meeting, the discussions were lively — sometimes heated — and the original time span allocated to the meeting was a result, comfortably exceeded by about 50%.作者: ingrate 時間: 2025-3-29 20:05
,Cosmic-Ray Acceleration and Transport, and Diffuse Galactic γ-Ray Emission,iew several source models, in particular supernovae exploding inside or near large interstellar clouds. The complex problem of cosmic ray transport in random electromagnetic fields is reduced to three cases which should be sufficient for practical purposes. As far as diffusive acceleration is concer作者: Discrete 時間: 2025-3-30 02:01
Acceleration and Transport Processes: Verification and Observations,r modulation of galactic cosmic rays and shock acceleration processes on the solar wind are examined and observational tests are summarized. It is concluded that the basic diffusive transport equation is a useful approximation in situations like the solar wind, where turbulent scattering by magnetic作者: 柔聲地說 時間: 2025-3-30 06:12 作者: 恫嚇 時間: 2025-3-30 11:38
Gamma Rays and Neutrinos as Complementary Probes in Astrophysics,mma rays, bring more readily information on high-energy electrons than on protons. Neutrinos provide a unique tracer for protons. Furthermore, at high energies the neutrino flux can considerably exceed the gamma-ray flux, as gamma rays above ~ 1 MeV are degraded by γ-γ interactions in compact high-i作者: 本土 時間: 2025-3-30 12:37
Gamma-Ray Sources Observed by Cos-B,ich appear point-like in the data, are mainly diffuse in nature or are genuinely compact objects. Most of the uncertainty is due to the experimental limitations. A status report is presented on the experimental study of the fine-scale structure measured by COS-B in the energy range 50 MeV-5 GeV. All作者: colostrum 時間: 2025-3-30 16:45
Point-Like Gamma-Ray Sources,oint sources. These models involve energetic processes associated with interstellar clouds, e.g. supernova-cloud interactions, neutron star accretion inside interstellar clouds, cloud collisions, etc. The dynamical evolution of such systems is discussed and physical processes are described in a math作者: 阻撓 時間: 2025-3-30 23:20
Gamma-Ray Pulsars in the MeV Region,ns can initiate electro-optical showers, which provide a secondary particle population at a lower energy. Both gamma and radio radiation are thought to be explicable within this framework..We show that — because of the properties of curvature radiation — there is an intrinsic lower limit to the gamm作者: 吸引人的花招 時間: 2025-3-31 01:16 作者: intricacy 時間: 2025-3-31 06:25
Gamma Rays from Close Binary Systems,n that high energy radiation should be efficiently produced at a shock front, where the pressure of the relativistic wind of the pulsar equals the ram pressure of the primary star wind. The expected number of such systems in the Galaxy is evaluated and the model is applied in some detail to the case作者: narcissism 時間: 2025-3-31 10:09
Gamma Rays from Active Regions in the Galaxy: The Possible Contribution of Stellar Winds,ferred to relativistic cosmic rays by diffusive shock acceleration at the wind boundary, and/or in the expanding, turbulent wind itself. Massive stars are most frequently found in OB associations, surrounded by H . regions lying at the edge of dense molecular clouds. The interaction of the freshly a作者: 木訥 時間: 2025-3-31 13:58 作者: 感染 時間: 2025-3-31 19:18
A Search for Counterparts of Selected Cos-B Galactic Gamma-Ray Sources: The X-Ray Survey and Opticaces discovered by the COS-B satellite..32 low latitude (|.| < 5°) IPC fields, mosaic-arranged to cover the few-square-degrees COS-B error circles, yielded 30 soft X-ray sources, the fluxes of which range from ~ 1/100 to few UFU, and no diffuse features..While the density of ~ 1 source/IPC field is c作者: Cardioplegia 時間: 2025-3-31 22:45 作者: 防止 時間: 2025-4-1 04:39
Origin of the Diffuse Galactic Gamma-Ray Emission at Low and Medium Gamma-Ray Energies,al measurements are now available at those energies, where the contribution from π°-decay gamma rays can be neglected. The high MeV-fluxes observed in both parts of the Galaxy are an indication of either a strong electron induced component or a high contribution from unresolved sources. Several inte作者: ALIEN 時間: 2025-4-1 07:48
The Use of Gamma Rays to Trace the Local Interstellar Hydrogen, from galaxy counts. It is found that to a good approximation the gamma-ray intensity is proportional to the total gas column density, and on this basis a map of the angular distribution of local molecular hydrogen at intermediate latitudes is presented. Comparing this with a simular map produced fr作者: 光亮 時間: 2025-4-1 12:20 作者: Fatten 時間: 2025-4-1 16:17
Comparison of Far-Infrared Radiation with Gamma Radiation,ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hum作者: Antimicrobial 時間: 2025-4-1 18:46
Conference proceedings 1983in Patras, August 19, 1982. Roughly one hundred scientists attended this meeting, the discussions were livel- sometimes heated - and the original time span allocated to the meeting was as a result, comfortably exceeded by about 50 % . The aim of this meeting was to determine the role of galactic gam作者: 連鎖,連串 時間: 2025-4-2 00:28
IAU, held in Patras, August 19, 1982. Roughly one hundred scientists attended this meeting, the discussions were livel- sometimes heated - and the original time span allocated to the meeting was as a result, comfortably exceeded by about 50 % . The aim of this meeting was to determine the role of ga作者: 確認 時間: 2025-4-2 06:44
