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Mixing in star-forming clouds explains why sibling stars look alike(图)
sibling star-forming clouds
2014/9/12
The chemical uniformity of stars in the same cluster is the result of turbulent mixing in the clouds of gas where star formation occurs, according to a study by astrophysicists at the University of Ca...
Herschel/HerMES: The X-ray - Infrared correlation for star-forming galaxies at z~1
X-ray - Infrared correlation star-forming galaxies
2011/9/29
For the first time, we investigate the X-ray/infrared (IR) correlation for star-forming galaxies at z~1, using SPIRE submm data from the recently-launched Herschel Space Observatory and deep X-ray dat...
Dissecting high-mass star-forming regions; tracing back their complex formation history
high-mass star-forming regions tracing complex formation
2011/9/26
We present near-infrared JHKs imaging as well as K-band multi-object spectroscopy of the massive stellar content of W3 Main using LUCI at the LBT. We confirm 13 OB stars by their absorption line spect...
Stellar masses of star-forming galaxies at 0.3 < z < 1.2 in the GOYA survey
Stellar masses star-forming galaxies .3 < z < 1.2
2009/6/18
Stellar masses of star-forming galaxies at 0.3 < z < 1.2 in the GOYA survey。
Lambda Orionis Star Forming Region:toward a comprehensive study of the stellar and substellar population
Lambda Orionis Star Forming Region substellar population
2009/6/18
Lambda Orionis Star Forming Region:toward a comprehensive study of the stellar and substellar population。