Results 261 to 270 of about 56,054 (306)

The star forming history on massive star forming region W51

, 1997
openaire   +1 more source

First submillimeter lights from Dome A: Tracing the carbon cycle in the feedback of massive stars. [PDF]

Sci Adv
Gong Y, Zhong J, Ren Y, Zhang Y, Liu D, Ao Y, Yao Q, Zhang W, Miao W, Lin Z, Duan W, Liu D, Zhou K, Liu J, Wang Z, Jin J, Zhang K, Wu F, Li J, Liu B, Zhang X, Luo Z, Wang J, Hao H, Lu X, Xie S, Quan J, Liu Y, Liang J, Deng X, Jiang J, Li L, Guo L, Ji T, Jiang P, Zhang Y, Shu C, Neupane S, Mao R, Shi S, Li J.   +40 more
europepmc   +1 more source

Dynamics and energy encoding of a star-like neuron network composed of the Wang-Zhang model induced by compressing a sphere into a fingertip. [PDF]

Cogn Neurodyn
Shi X, Xu W, Zhuang L, Meng F, Jiang H, Wang Z.   +5 more
europepmc   +1 more source

Immersive virtual reality for cognitive rehabilitation in patients who had a stroke: study protocol for a randomised controlled trial. [PDF]

BMJ Open
Li JL, Meng FL, Ma J, Wu JJ, He S, Zhang JP, Xu ZJ, Zheng YX, Mei YD, Hua XY, Xu JG.   +10 more
europepmc   +1 more source

Evolution of Southern Star-Forming Regions

Astrophysics and Space Science, 1997
We present ISO observations of bright, high-mass southern star-forming regions with the Short Wavelength Spectrometer (SWS) and Long Wavelength Spectrometer (LWS). The selected targets show a range of pre-main sequence evolutionary phases. Whereas some objects still show interstellar ice features, the most evolved objects are coincident with ...
Ehrenfreund, P., Dishoeck, E.F., Burgdorf, M., Cami, J., van Hoof, P.A.M., Tielens, A.G.G.M., Schutte, W.A., Thi, W.F.D.   +7 more
openaire   +4 more sources

Investigating the structure of star-forming regions using INDICATE [PDF]

Monthly Notices of the Royal Astronomical Society, 2022
The ability to make meaningful comparisons between theoretical and observational data of star-forming regions is key to understanding the star formation process.
George A Blaylock-Squibbs, Richard J Parker, Anne S M Buckner   +2 more
exaly   +2 more sources

Dynamical evolution of fractal structures in star-forming regions [PDF]

Monthly Notices of the Royal Astronomical Society, 2020
The Q-parameter is used extensively to quantify the spatial distributions of stars and gas in star-forming regions as well as older clusters and associations.
Emma C Daffern-Powell, Richard J Parker, Parker Richard J   +2 more
exaly   +2 more sources

Implications of the kinematical structure of circumnuclear star-forming regions on their derived properties [PDF]

Monthly Notices of the Royal Astronomical Society, 2013
We review the results of high-dispersion spectroscopy of 17 circumnuclear star-forming regions (CNSFRs) in 3 nearby early spiral galaxies, NGC 2903, NGC 3310 and NGC 3351.
G F Hagele, Angeles I Diaz, Roberto Terlevich   +2 more
exaly   +1 more source

The dynamical evolution of star-forming regions measured with INDICATE [PDF]

Monthly Notices of the Royal Astronomical Society
Observations of star-forming regions provide snapshots in time of the star formation process, and can be compared with simulation data to constrain the initial conditions of star formation.
George A Blaylock-Squibbs, Richard J Parker, Parker Richard J   +2 more
exaly   +4 more sources

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Chemistry of Star-Forming Regions

The Journal of Physical Chemistry A, 2005
The space between stars is not empty but contains gas-phase and particulate matter under varying conditions. Neutral matter is found mainly in large regions of the interstellar medium known as "clouds", the largest of which, termed "giant molecular clouds", are essentially molecular in nature.
openaire   +2 more sources