机译:NGC 1851红巨型分支和渐近巨人分支星星:四边形分布
Monash Centre for Astrophysics P.O. Box 28M Victoria 3800 Australia;
Research School of Astronomy and Astrophysics Australian National University Weston ACT 2611 Australia;
Research School of Astronomy and Astrophysics Australian National University Weston ACT 2611 Australia;
Monash Centre for Astrophysics P.O. Box 28M Victoria 3800 Australia;
Monash Centre for Astrophysics P.O. Box 28M Victoria 3800 Australia;
Monash Centre for Astrophysics P.O. Box 28M Victoria 3800 Australia;
Monash Centre for Astrophysics P.O. Box 28M Victoria 3800 Australia;
Australian Astronomical Observatory North Ryde NSW 2113 Australia;
Department of Physics and Astronomy Aarhus University Ny Munkegade DK-8000 Aarhus C Denmark;
Department of Astronomy and McDonald Observatory University of Texas Austin TX 78712 United States;
globular clusters: general - globular clusters: individual (NGC 1851; NGC 288)-stars:AGB and post-AGB;
机译:NGC 1851红巨型分支和渐近巨人分支星星:四边形分布
机译:NGC 205的渐近巨型分支:从JHK图像中识别出的碳星和巨星的特征
机译:NGC 205的渐近巨分支:从JHK影像中识别出的碳星和M巨星的特征
机译:红外研究在麦哲伦云中一些最糊涂的渐近巨星星星的变异性和大众损失
机译:Spitzer研究麦哲伦星云中渐近巨分支恒星的质量损失和红外变异性。
机译:玉米淀粉分支酶同工型和支链淀粉结构。在缺乏淀粉分支酶IIb的情况下,进一步缺乏淀粉分支酶Ia会导致分支增加
机译:二元恒星的绝热质量损失。 III。从红巨型分支的底部到渐近巨型分支的尖端
机译:渐近巨星支星的红外研究