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Red Giant Survival

Scientific American, 2007
This article reports that astronomers have found an exoplanet that likely survived the red giant phase of its parent star. Named V391 Pegasi, it belongs to a class of subdwarf stars that flicker. Researchers noticed the regularity of the flickering and says it is a planet at least 3 times bigger than Jupiter.
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Rotation of Red Giants

EAS Publications Series, 2015
A new rotation model for post-main sequence stars is proposed. This model quantitatively reproduces core and surface rotation rates of subgiant stars, as well as the core rotation of helium-burning clump stars.
Y. Kissin, C. Thompson
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Axion bremsstrahlung in red giants

Physical Review D, 1990
We calculate the bremsstrahlung emission rate of axions from a degenerate but weakly coupled plasma, using a Debye structure factor to take account of the nuclei correlations. This result pertains to axion emission from red giants near the helium flash and thus could be used to make a previous bound precise which involves the suppression of helium ...
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Chromospheres in Red Giants

1994
Increasing evidence suggests that the mechanism(s) for heating the chromospheres of the coolest red giants may be quite different from those responsible for heating in solar-type stars, but little progress toward a quantitative test of this important idea has been made, both because of the scarcity of suitable observations and the difficulty of ...
Hollis R. Johnson   +2 more
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Red Giant Masers

1981
Basic concepts in the theory of astronomical masers which are necessary for the discussion of red giant masers are introduced. Maser radiation from late type stars is then discussed in detail with special emphasis on SiO masers as probes of the stellar atmosphere and OH masers as a tool for studying the mass loss process and the circumstellar shell.
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Winds in Red Giants

1981
Expanding, cool envelopes around red giants were detected many years ago when Adams and McCormack (1935) discovered that on high dispersion spectra of ∝ Ori, ∝1 Her, o Cet and e Peg the stronger resonance lines showed violet displaced absorption cores which could be explained by an expanding gaseous envelope.
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Fred Hoyle, Red Giants and Beyond

Astrophysics and Space Science, 2003
The impact of Fred Hoyle’s work on the structure and evolution of red giants, particularly his breakthrough contribution with Martin Schwarzschild (1955), is described and assessed. Working with his students in the early 1960s, Hoyle presented new physical ways of understanding some of the approximations used, and results obtained, in that seminal ...
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Giant virus biology and diversity in the era of genome-resolved metagenomics

Nature Reviews Microbiology, 2022
Frederik Schulz   +2 more
exaly  

Structural Chemistry of Giant Metal Based Supramolecules

Chemical Reviews, 2021
Alexander V Virovets   +2 more
exaly  

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