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《Nature Astronomy》发表广州大学物理与材料科学学院陈曦团队新种类分子脉泽与大质量恒星形成的重要研究成果（图）
广州大学物理与材料科学学院 Nature Astronomy 陈曦 天体脉泽 大质量恒星
2020/7/27
近日，广州大学物理与材料科学学院陈曦教授及其国际合作团队，在天体脉泽与大质量恒星形成研究方向取得重要突破，论文于北京时间 2020 年 7 月 14 日在线发表于《 Nature Astronomy 》（自然 - 天文学）。该期刊是英国著名杂志《自然》于 2017 年创立的自然科学类子刊， 是天文学领域国际权威学术期刊。
The Nature of Star Formation at 24 microns in the Group Environment at 0.3 < z < 0.55
Nature Star Formation Group Environment
2011/10/8
Galaxy star formation rates (SFRs) are sensitive to the local environment; for example, the high-density regions at the cores of dense clusters are known to suppress star formation. It has been sugges...
Distance determination for RAVE stars using stellar models III: The nature of the RAVE survey and Milky Way chemistry
Stars: distances, Stars: fundamental parameters, Galaxy: abundances, Galaxy: disk, Galaxy: stellar content, Galaxy: structure
2011/9/29
We apply the method of Burnett & Binney (2010) for the determination of stellar distances and parameters to the internal catalogue of the Radial Velocity Experiment (Steinmetz et al. 2006). Subsamples...
On the nature of the open clusters in the direction of ngc 6882/5
open clusters ngc 6882/5
2009/7/10
On the nature of the open clusters in the direction of ngc 6882/5。
Exploring the nature of weak Chandra sources near the Galactic centre
weak Chandra sources Galactic centre
2009/6/17
Exploring the nature of weak Chandra sources near the Galactic centre。
Revealing the nature of the highly obscured galactic Source igr j16318-4848
highly obscured galactic Source igr j16318-4848
2009/6/17
Revealing the nature of the highly obscured galactic Source igr j16318-4848。
The nature of the very extended emission line regions associated with active galactic nuclei
emission line regions active galactic nuclei
2009/6/11
The nature of the very extended emission line regions associated with active galactic nuclei。
Unravelling the Nature of HD 81032 – A New RS CVn Binary
Star-X-ray star-variable star-late-type star-HD 81032
2009/5/12
BVR photometric and quasi-simultaneous optical spectroscopic
observations of the star HD81032 have been carried out during
the years 2000–2004. A photometric period of 18.802 ± 0.07d has been
dete...