Results 31 to 40 of about 2,275,942 (365)
Carbon-deficient Red Giants [PDF]
Abstract Carbon-deficient red giants (CDRGs) are a rare class of peculiar red giants, also called “weak G-band” or “weak CH” stars. Their atmospheric compositions show depleted carbon, a low isotopic ratio, and an overabundance of nitrogen, indicating that the material at ...
Howard E. Bond, Howard E. Bond
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TESS asteroseismology of the Kepler red giants [PDF]
ABSTRACTRed giant asteroseismology can provide valuable information for studying the Galaxy as demonstrated by space missions like CoRoT and Kepler. However, previous observations have been limited to small data sets and fields of view. The TESS mission provides far larger samples and, for the first time, the opportunity to perform asteroseimic ...
Stello, Dennis+13 more
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Characterization of the gut microbiota in the red panda (Ailurus fulgens). [PDF]
The red panda is the only living species of the genus Ailurus. Like giant pandas, red pandas are also highly specialized to feed mainly on highly fibrous bamboo.
Fanli Kong+9 more
doaj +1 more source
The brightness of the tip of the red-giant branch (TRGB) allows one to constrain novel energy losses that would lead to a larger core mass at helium ignition and thus to a brighter TRGB than expected by standard stellar models. The required absolute TRGB
F. Capozzi, G. Raffelt
semanticscholar +1 more source
Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Redetermination of the Hubble Constant [PDF]
We present a calibration of the tip of the red giant branch (TRGB) in the Large Magellanic Cloud (LMC) on the Hubble Space Telescope (HST)/ACS F814W system.
W. Yuan+4 more
semanticscholar +1 more source
AbstractThe longest-known class of pulsating variable stars, namely pulsating red giants, is also the one that involves the most complex physical processes. Pulsation, mass loss, nuclear synthesis, mixing, atmospheric and circumstellar chemistry and dust formation all interrelate with one another and make both the observational studies and the ...
Franz Kerschbaum, Walter Nowotny
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Illumination in symbiotic binary stars: Non-LTE photoionization models. II. Wind case [PDF]
We describe a non-LTE photoionization code to calculate the wind structure and emergent spectrum of a red giant wind illuminated by the hot component of a symbiotic binary system.
Almog Y.+34 more
core +3 more sources
Core rotation braking on the red giant branch for various mass ranges [PDF]
Context. Asteroseismology allows us to probe stellar interiors. In the case of red giant stars, conditions in the stellar interior are such as to allow for the existence of mixed modes, consisting in a coupling between gravity waves in the radiative ...
C. Gehan+4 more
semanticscholar +1 more source
The changes in the expression of genes related to digestion and metabolism may be various in different dietary mammals from juvenile to adult, especially, the giant panda (Ailuropoda melanoleuca) and red panda (Ailurus fulgens), which were once ...
Zhuma Yizhen+9 more
doaj +1 more source
Weighing the stellar constituents of the galactic halo with APOGEE red giant stars [PDF]
The stellar mass in the halo of the Milky Way is notoriously difficult to determine, owing to the paucity of its stars in the solar neighbourhood. With tentative evidence from Gaia that the nearby stellar halo is dominated by a massive accretion event –
J. Mackereth, J. Bovy
semanticscholar +1 more source