机译:来自尘埃稀少且分子气体少的区域的两次γ射线
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;
Department of Astronomy, Kyoto University, Kyoto 606-8502, Japan;
Kavli Institute of NanoScience, Faculty of Applied Sciences, Delft University of Technology, Lorentzweg 1, 2628 CJ Delft, The Netherlands;
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan,Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura, Santiago 763 0355, Chile,The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;
Institute of Astronomy, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan;
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;
Institute of Astronomy, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan,Research Centre for the Early Universe, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan;
机译:赫歇尔对伽马射线爆发宿主星系的观测:对尘土飞扬的星际介质拓扑结构的影响
机译:尘埃Mg II吸收剂:对伽马射线爆炸/准星入射差异的影响
机译:天然H II区的氦气:伽玛射线爆炸后X射线吸收的起源
机译:Gamma射线从尘土飞扬的地区爆发,少量分子气体
机译:伽马射线暴/超新星连接,伽马射线暴的距离估算器以及对伽马射线暴余辉进行建模。
机译:活动星系核遮蔽不受风暴:从DUsTY红外驱动以温暖和X射线光电离
机译:Gamma射线从尘土飞扬的地区爆发,少量分子气体
机译:星形成区域的X射线瞬变和X射线爆发的“硬X射线发射”