图书简介
Perseus is an outstanding case in which to study the physics of relativistic plasma and thermal gas, and the interplay between galactic nuclei and galaxy clusters. Ground and space observatories have recently provided some ground-breaking insights into the Perseus system, from a detailed image of a jet launched in the vicinity of a supermassive black hole, through VLBI, to an unexpected degree of turbulence in the cluster core, constrained by high energy resolution in x-rays. While preparing for the next generation observatories that will allow readers to address these questions in other systems, this volume provides some first steps in exploring topics relating to particle acceleration, energy transport between large and small scales and the role of magnetic fields in the launch of relativistic jets. Chapters deal with the latest results covering theory, observations, and numerical simulations, spanning a wide range in physical scales and energy ranges.
Preface; Editors; Participants; Black hole mass measurements in AGN: Polarization in broad emission lines; Fully analytical solutions for Bondi accretion in galaxies with a central Black; Modelling the polarised emission from black holes on event horizon-scales; Particle acceleration and the origin of the very high energy emission around black holes and relativistic jets; Numerical methods for general relativistic particles; On the prospects of imaging Sagittarius A* from space; The Hot Universe with XRISM and Athena; Low frequency observations of radio relics and halos; Probing the non-thermal emission in the Perseus cluster with the JVLA; High-dynamic-range 21 cm JVLA observations of the Perseus Cluster; A wide and collimated radio jet in 3C 84; Extragalactic relativistic jets; Inflow and outflow (Jets) in NGC 1275; Observations of nearby relativistic jets with EAVN and EATING VLBI; Molecular gas filamentary structures in galaxy clusters; Young radio jets breaking free: molecular and HI outflows in their centers; Ultrafast outflows, and their connection to accretion and ejection processes in AGNs; AGN feedback and the origin and fate of the hot gas in early-type galaxies; Numerical study of active galactic nucleus feedback in an elliptical galaxy with MACER; Prodigious and continuous formation of super star clusters from cooled intracluster gas; Characterizing the outburst of the supermassive black hole in M87; X-ray probing of NGC 1275 nuclear region with Hitomi, Swift, and Suzaku; Life-cycles and energetics of radio-loud AGN; Deep Chandra observations of the core of the Perseus cluster; Close-up view of an ongoing merger between the NGC 4839 group and the Coma cluster; Thermal and non-thermal connection in radio mini-halos; Perseus: a huge reservoir of dark matter investigated with MAGIC; The AGN dependence on cluster mass; AGN jets, bubbles, and heat pumps; Intermediate-mass black hole feedback in dwarf galaxies: a view from cosmological simulations; Gamma-ray emission in radio galaxies, from MeV to TeV; Search for QPOs in Perseus with Fermi LAT; High energy ?-ray variability of NGC 1275 and 3C 120; Young radio sources at high-energies and the ?-ray CSO PKS 1718?649; Exploring the radio and GeV-TeV ?-ray connection in the different blazar sub-classes; Neutrino and ?-ray emission from the core of NGC1275 by magnetic reconnection: GRMHD simulations and radiative transfer/particle calculations; Magnetic fields in the relativistic jets of active galactic nuclei; The correlation between the total jet power and the Poynting flux at the jet base; Why only a small fraction of quasars are radio loud?; Ratio of kinetic-to-bolometric luminosity at the ?cold? disk accretion onto black holes; Emission modelling of hydrodynamic AGN jet simulations; The wind production from black hole hot accretion flow; Radio-loud AGNs with peculiar shape of hard X-ray spectrum: figuring out the reasons; Expanding radio lobe associated with 3C 84; Chandra view on the active nucleus of CGCG292?057: Jet-ISM interactions; Preliminary analysis of the X-ray emission from the central regions of the Pictor; Flip of the jet head position of 3C 84 in 2015; AGN and star formation feedback in galaxy outflows; Update on the multi-frequency monitoring of blazars with Medicina and Noto; Hints of radio sources evolution; Bending of the pc scale jet in 3C84; Chandra early-type galaxy atlas; Probing the B-fields of AGN jets on kiloparsec scales ? NGC 6251; External blob radiation model for the TeV gamma-ray emission in radio galaxies; A negative correlation between RUV and ?OX in low-luminosity AGNs; A precessing and nutating jet in OJ287; A jet proper motion study in the early Universe; Evolution of the M? ? ? relation; Simulations of the W50-SS433 system; Black hole demographics from TDE modeling; Multi-frequency monitoring of S5 0716+714; Survival of populat
Trade Policy 买家须知
- 关于产品:
- ● 正版保障:本网站隶属于中国国际图书贸易集团公司,确保所有图书都是100%正版。
- ● 环保纸张:进口图书大多使用的都是环保轻型张,颜色偏黄,重量比较轻。
- ● 毛边版:即书翻页的地方,故意做成了参差不齐的样子,一般为精装版,更具收藏价值。
关于退换货:
- 由于预订产品的特殊性,采购订单正式发订后,买方不得无故取消全部或部分产品的订购。
- 由于进口图书的特殊性,发生以下情况的,请直接拒收货物,由快递返回:
- ● 外包装破损/发错货/少发货/图书外观破损/图书配件不全(例如:光盘等)
并请在工作日通过电话400-008-1110联系我们。
- 签收后,如发生以下情况,请在签收后的5个工作日内联系客服办理退换货:
- ● 缺页/错页/错印/脱线
关于发货时间:
- 一般情况下:
- ●【现货】 下单后48小时内由北京(库房)发出快递。
- ●【预订】【预售】下单后国外发货,到货时间预计5-8周左右,店铺默认中通快递,如需顺丰快递邮费到付。
- ● 需要开具发票的客户,发货时间可能在上述基础上再延后1-2个工作日(紧急发票需求,请联系010-68433105/3213);
- ● 如遇其他特殊原因,对发货时间有影响的,我们会第一时间在网站公告,敬请留意。
关于到货时间:
- 由于进口图书入境入库后,都是委托第三方快递发货,所以我们只能保证在规定时间内发出,但无法为您保证确切的到货时间。
- ● 主要城市一般2-4天
- ● 偏远地区一般4-7天
关于接听咨询电话的时间:
- 010-68433105/3213正常接听咨询电话的时间为:周一至周五上午8:30~下午5:00,周六、日及法定节假日休息,将无法接听来电,敬请谅解。
- 其它时间您也可以通过邮件联系我们:customer@readgo.cn,工作日会优先处理。
关于快递:
- ● 已付款订单:主要由中通、宅急送负责派送,订单进度查询请拨打010-68433105/3213。
本书暂无推荐
本书暂无推荐