机译:大规模螺旋星系的热凝航介质的Baryon预算
Department of Astronomy University of Michigan 311 West Hall 1085 South University Avenue Ann Arbor MI 48109-1107 USA;
Department of Astronomy University of Michigan 311 West Hall 1085 South University Avenue Ann Arbor MI 48109-1107 USA;
Department of Astronomy University of Massachusetts 710 North Pleasant Street Amherst MA 01003 USA;
Astrophysics Research Institute Liverpool John Moores University IC2 Liverpool Science Park 146 Brownlow Hill Liverpool L3 5RF UK;
Max-Planck Institute for Astrophysics Karl-Schwarzschild-Straβe 1 D-85748 Garching bei München Germany;
intergalactic medium; galaxies: evolution; galaxies: fundamental parameters; galaxies: halos; galaxies: spiral; X-rays: galaxies;
机译:大规模螺旋星系的热凝航介质的Baryon预算
机译:三个QSO的HST / COS谱图探测单个螺旋银河的环流介质:气体再循环和流出的证据*
机译:100千帕秒的风向巨大的紧凑星系的绕银河系介质供气
机译:集线器:专用的热凝固型媒介探险家
机译:通过银河-麦哲伦系统的绕银河介质中的重子流进行的现代银河演化
机译:星系团冷热重子的反相关检测
机译:大螺旋的环银河系媒介。二。探索最庞大的孤立螺旋星系周围的热气态晕的性质