Results 121 to 130 of about 3,957,653 (321)
Stellar Winds on the Main-Sequence I: Wind Model
Aims: We develop a method for estimating the properties of stellar winds for low-mass main-sequence stars between masses of 0.4 and 1.1 solar masses at a range of distances from the star.
Brott, I.+4 more
core +2 more sources
Evolution of Stars of Small Masses in the Pre-Main-Sequence Stages [PDF]
Chûshirô Hayashi, Takenori Nakano
openalex +1 more source
Transcriptome‐wide analysis of circRNA and RBP profiles and their molecular relevance for GBM
CircRNAs are differentially expressed in glioblastoma primary tumors and might serve as therapeutic targets and diagnostic markers. The investigation of circRNA and RNA‐binding proteins (RBPs) interactions shows that distinct RBPs play a role in circRNA biogenesis and function.
Julia Latowska‐Łysiak+14 more
wiley +1 more source
A Test Of Pre-Main-Sequence Lithium Depletion Models [PDF]
Despite the extensive study of lithium depletion during pre-main-sequence (PMS) contraction, studies of individual stars show discrepancies between ages determined from the Hertzsprung-Russell (H-R) diagram and ages determined from lithium depletion ...
Jensen, Eric L.N.+1 more
core +1 more source
Rotation and activity of pre-main-sequence stars
We present a study of rotation (vsini) and chromospheric activity (Halpha EW) based on an extensive set of high-resolution optical spectra obtained with MIKE on the 6.5m Magellan Clay telescope.
Alexander Scholz+12 more
core +1 more source
Magnetic Fields in Stellar Bodies: II. Magnetic Fields in Upper Main Sequence Stars [PDF]
J. J. Monaghan
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Combining melting curve analysis enhances the multiplexing capability of digital PCR. Here, we developed a 14‐plex assay to simultaneously measure single nucleotide mutations and amplifications of KRAS and GNAS, which are common driver genes in pancreatic cancer precursors. This assay accurately quantified variant allele frequencies in clinical samples
Junko Tanaka+10 more
wiley +1 more source
Half a Million Binary Stars Identified from the Low-resolution Spectra of LAMOST
Binary stars are prevalent yet challenging to detect. We present a novel approach using convolutional neural networks (CNNs) to identify binary stars from low-resolution spectra obtained by the LAMOST survey.
Yingjie Jing+4 more
doaj +1 more source
Atmospheric velocity fields in tepid main sequence stars
The line profiles of the stars with v sin i below a few km/s can reveal direct signatures of local velocity fields (e.g. convection) in stellar atmospheres. This effect is well established in cool main sequence stars, and has been detected and studied in
A. Townshend+41 more
core +2 more sources
The Pulsational Properties of an Early Main-Sequence Star, I [PDF]
H. S. Gurm
openalex +1 more source