Results 181 to 190 of about 180,740 (304)
Cosmological Implications of He-3 Destruction on the Red Giant Branch
Arnold I. Boothroyd, Robert Malaney
openalex +2 more sources
The Shape of the Red Giant Branch Bump as a Diagnostic of Partial Mixing Processes in Low‐Mass Stars [PDF]
S. Cassisi, M. Salaris, G. Bono
openalex +1 more source
ABSTRACT Traditional leaf gas exchange experiments have focused on net CO2 exchange (Anet). Here, using California poplar (Populus trichocarpa), we coupled measurements of net oxygen production (NOP), isoprene emissions and δ18O in O2 to traditional CO2/H2O gas exchange with chlorophyll fluorescence, and measured light, CO2 and temperature response ...
Kolby Jeremiah Jardine+8 more
wiley +1 more source
Revisiting the Activity–Rotation Relation for Evolved Stars
The magnetic dynamo mechanism of giant stars remains an open question, which can be explored by investigating their activity–rotation relations with multiple proxies. By using the data from the LAMOST and Galaxy Evolution Explorer surveys, we carried out
Henggeng Han+4 more
doaj +1 more source
First Detection of the Red Giant Branch Bump in the Sagittarius Dwarf Spheroidal Galaxy [PDF]
L. Monaco+3 more
openalex +1 more source
Measuring the core rotation of red giant stars
Red giant stars present mixed modes, which behave as pressure modes in the convective envelope and as gravity modes in the radiative interior. This mixed character allows to probe the physical conditions in their core.
Gehan, Charlotte+2 more
core
SUMMARY The dinoflagellate family Amphidomataceae includes the genera Azadinium and Amphidoma, several species of which are known producers of lipophilic toxins known as azaspiracids (AZAs). However, the diversity, abundance, and distribution of this important group of nanoplanktonic dinoflagellates in the Black Sea remain poorly understood. To address
Urban Tillmann+5 more
wiley +1 more source
Mining the GALAH Data. I. Study of Five Super Lithium-rich Metal-poor Giants
The presence of a large amount of Li in giants is still a mystery. Most of the super Li-rich (SLR) giants reported in recent studies are in the solar metallicity regime.
Antony Susmitha+2 more
doaj +1 more source
Why hot horizontal branch stars can appear redder than red giants [PDF]
Y. Momany+6 more
openalex +1 more source
`\delta \mu mixing' on the Red Giant Branch [PDF]
Graeme H. Smith+7 more
openaire +1 more source