Results 61 to 70 of about 2,275,942 (365)

On the serendipitous discovery of a Li-rich giant in the globular cluster NGC 362 [PDF]

open access: yes, 2015
We have serendipitously identified the first lithium-rich giant star located close to the red giant branch bump in a globular cluster. Through intermediate-resolution FLAMES spectra we derived a lithium abundance of A(Li)=2.55 (assuming local ...
Angelou, George C.   +8 more
core   +2 more sources

Red giants seismology

open access: yes, 2013
SF2A 2013 ...
Mosser, Benoît   +2 more
openaire   +4 more sources

Occurrence of the red giant flying squirrel (Petaurista petaurista: Sciuridae) in Bangladesh

open access: yesNature Conservation Research: Заповедная наука, 2018
This report confirms the presence of the red giant flying squirrel Petaurista petaurista from the Idgarh Reserve Forest in Cox's Bazar (North) Forest Division in the southern part of Bangladesh. The chestnut-red dorsal body colour, white ventral surface,
M. Tarik Kabir   +3 more
doaj   +1 more source

Oscillations in g-mode period spacings in red giants as a way to determine their state of evolution

open access: yesEPJ Web of Conferences, 2015
In this work we consider the sensitivity of gravity-mode period spacings to sharp changes in the inner structure of red giant stars, more specifically in the buoyancy frequency inside the g-mode propagation cavity.
Cunha M. S.   +3 more
doaj   +1 more source

Infrared Spectroscopy of Symbiotic Stars. IV. V2116 Ophiuchi/GX 1+4, The Neutron Star Symbiotic [PDF]

open access: yes, 2005
We have computed, based on 17 infrared radial velocities, the first set of orbital elements for the M giant in the symbiotic binary V2116 Ophiuchi. The giant's companion is a neutron star, the bright X-ray source GX 1+4. We find an orbital period of 1161
Bandyopadhyay R.   +26 more
core   +4 more sources

The brightness of the Red Giant Branch tip: Theoretical framework, a set of reference models, and predicted observables [PDF]

open access: yes, 2017
The brightness of the tip of the Red Giant Branch is a useful reference quantity for several fields of astrophysics. An accurate theoretical prediction is needed for such purposes. Aims.
A. Serenelli   +8 more
semanticscholar   +1 more source

Fingering convection in red giants revisited [PDF]

open access: yesAstronomy & Astrophysics, 2014
Accepted for publication in Astronomy and ...
Sylvie Vauclair   +3 more
openaire   +6 more sources

Gene expressions between obligate bamboo-eating pandas and non-herbivorous mammals reveal converged specialized bamboo diet adaptation

open access: yesBMC Genomics, 2023
Background It is inevitable to change the function or expression of genes during the environmental adaption of species. Both the giant panda (Ailuropoda melanoleuca) and red panda (Ailurus fulgens) belong to Carnivora and have developed similar ...
Jinnan Ma   +10 more
doaj   +1 more source

KOI-3890: A high mass-ratio asteroseismic red-giant$+$M-dwarf eclipsing binary undergoing heartbeat tidal interactions [PDF]

open access: yes, 2019
KOI-3890 is a highly eccentric, 153-day period eclipsing, single-lined spectroscopic binary system containing a red-giant star showing solar-like oscillations alongside tidal interactions.
Bell, Keaton J.   +11 more
core   +3 more sources

On the Correlation Between Metallicity and the X-Shaped Morphology of the Milky Way Bulge

open access: yes, 2014
We demonstrate that failure to properly account for stellar evolution can bias results in determinations of the spatial morphology of Galactic bulge stars, focusing on the question of whether or not the X-shape is more pronounced among the more metal ...
Athanassoula, E.   +2 more
core   +3 more sources

Home - About - Disclaimer - Privacy