CRESST and X-ray Astrophysics Laboratory NASA/GSFC, Greenbelt, MD 20771 Department of Physics, University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250;
Observatoire astronomique de Strasbourg, Universite de Strasbourg, CNRS, INSU, 11 rue de l'universite,67000 Strasbourg, Prance;
Rochester Institute of Technology, 54 Lomb Memorial Drive, Rochester, NY 14623;
Vanderbilt University, Nashville, TN 37235;
Rochester Institute of Technology, 54 Lomb Memorial Drive, Rochester, NY 14623;
stars; formation — stars; individual (V1647 Ori) — stars; pre-main-sequence — X-rays; stars;
机译:迅速成长的年轻恒星发出X射线爆发,照亮了麦克尼尔的星云
机译:麦克尼尔星云的发光之星V1647 ORI的爆炸后红外光谱
机译:麦克尼尔星云的发光之星V1647 ORI的爆炸后红外光谱
机译:Suzaku观察来自Accreding的年轻明星的新X射线爆发,照亮McNeil的星云
机译:积聚的中子星和黑洞的X射线和光学观察以及恒星X射线旋光仪的构造和测试。
机译:最活跃的年轻恒星的绕星盘
机译:V1647 Ori(爆发后的年轻恒星照亮了麦克尼尔的星云)增强了X射线的可变性
机译:来自快速吸收年轻恒星的X射线爆发照亮了麦克尼尔的星云