3
...Some carbon-rich evolved stars exhibit a very prominent spectral feature at ~"30 μm." The C-rich...
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4
by Tian, Feng
Published 2015
... Earths (6-10 Earth masses) in the habitable zones of typical low-mass M stars to the enhanced soft X-ray...
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5
by Polishook, David
Published 2015
...The nearby Type Ia supernova (SN Ia) SN 2011fe in M101 (cz = 241 km s[superscript –1]) provides a...
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6
...We report the detection of 24 μm variations from the planet-hosting υ Andromedae system consistent...
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9
... investigate here the potential of this approach for the M dwarf GJ 1214 that hosts a transiting super-Earth...
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16
... submesoscale water-mass variability in the seasonal pycnocline at 20–60-m depths. To filter out internal waves...
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17
... sizes (<2 μm) similar to those found in CP IDPs, we used a radiative transfer code adapted for light...
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