图书简介
This volume, the proceedings of IAU Symposium 363, addresses the astrophysical implications of gravitational wave and electromagnetic observations of neutron stars. It covers the state of the art understanding of mergers of binary neutron stars producing short gamma-ray bursts, and the most powerfully magnetic varieties of neutron stars, magnetars. Encapsulating both observations and modelling, the contributions address extreme transient events including kilonovae, afterglows, magnetar giant flares, and fast radio bursts. By exploring the intersection of studies of isolated neutron stars and binary system synthesis and merging, this collection sets the scene for interpreting exciting results pertaining to powerful x-ray, gamma-ray, and gravitational wave transients to be acquired in the next decade and beyond. IAU S363 will be an asset for astronomers seeking a broad and interdisciplinary overview of neutron stars, their gravitational waves and electromagnetic emission.
Part I. The Search for Continuous Gravitational Waves; Part II. Exploring the Neutron Star Zoo; Part III. Observations of gravitational-wave afterglows Alessandra Corsi; GRB 170817A and the long-term aftermath of neutron star mergers Hendrik van Eerten; Kilonovae and short GRBs observations in the multi-messenger era Paolo D’Avanzo; Modeling kilonova emission from neutron star mergers Masaomi Tanaka; Multi-messenger science with Athena and future multi-messenger observatories Luigi Piro; Part IV. Physics in Ultra-Strong Magnetic Fields Alice Harding; Magnetic field evolution in the crust of neutron stars; Part IV. Physics in Ultra-Strong Magnetic Fields Alice Harding; Magnetic field evolution in the crust of neutron stars; Part V. Search for gravitational-wave transients associated with magnetar bursts during the third Advanced LIGO and Advanced Virgo observing run Kara Merfeld; Inferring the dense nuclear matter equation of state with neutron star tides Pantelis Pnigouras; Constraining three-nucleon forces with multimessenger data Andrea Sabatucci; Modelling the deformability of magnetized neutron stars in the light of future continuous gravitational waves detection Niccolo Bucciantini; Prospects for studying Galactic neutron stars in binaries with LISA Valeriya Korol; Gravitational-wave EM Counterpart Korean Observatory (GECKO) Myungshin Im; The neutron star neutron star merger GW170817; part Korean Observatory (GECKO) Myungshin Im; The neutron star neutron star merger GW170817; Part VI. INTEGRAL contributions to magnetars and multimessenger astrophysics Sandro Mereghetti; PULXs as accreting magnetars.
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