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An AzTEC 1.1-mm survey for ULIRGs in the field of the Galaxy Cluster MS 0451.6-0305
late-type galaxies mid-IR galaxies
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2014/12/22
We have undertaken a deep (σ∼ 1.1 mJy) 1.1-mm survey of the z= 0.54 cluster MS 0451.6−0305 using the AzTEC camera on the James Clerk Maxwell Telescope. We detect 36 sources with signal-to-...
Excitation of Solar-like Oscillations：From PMS to MS Stellar Models
Turbulence convection oscillations excitation sun stars:α Cen A—stars:main and pre-main sequence stars
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2009/5/12
The amplitude of solar-like oscillations results from a balance
between excitation and damping. As in the sun, the excitation is attributed
to turbulent motions that stochastically excite the p mode...
SOME CORRELATIONS FOR MASSIVE MS STARS
MS STARS CORRELATIONS
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2009/4/16
SOME CORRELATIONS FOR MASSIVE MS STARS。
ON THE CONVECTIVE CORES OF MS ROTATING STARS
Stars interiors-Stars rotation
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2009/2/18
An analysis of the influence of the uniform stellar rotation on
masses and radii of convective cores of zero age stars is presented. The study also
shows the dependence of the relative mass of the c...