Results 101 to 110 of about 84,685 (303)
Chemical abundances in HII regions and temperature fluctuations
H II regions are essential tools for the study of the chemical composition and chemical evolution of the Universe, specially in the extragalactic domain.
García-Rojas, Jorge
core +1 more source
Loss of the miR‐214/199a cluster is associated with recurrence in ovarian cancer. Engineered small extracellular vesicles (m214‐sEVs) elevate miR‐214‐3p/miR‐199a‐5p in tumor cells, suppress β‐catenin, TLR4, and YKT6 signaling, reprogram tumor‐derived sEV cargo, reduce chemoresistance and migration, and enhance carboplatin efficacy and survival in ...
Weida Wang +12 more
wiley +1 more source
Chemical abundances in leading arm and stream
The Magellanic Stream and its Leading Arm provide an unparalleled opportunity to map out the chemical abundances in a gaseous tidal stream. UV absorption-line studies with the HST/COS spectrograph have confirmed that the two main filaments of the ...
Fox, Andrew (8180115), Fox, Andrew
core +1 more source
Interrogating the immune landscape of microsatellite stable RAS‐mutated colon cancer
COLOSSUS project RAS‐mutated MSS colon cancer study explored transcriptomics and immune cell density by immunohistochemistry (IHC), Immunoscore (IS), ISIC/TuLIS scores, mutation counts, and detected different prevalences but similar microenvironment composition across immune markers with clinical relevance for future immunotherapy combination ...
Rodrigo Dienstmann +61 more
wiley +1 more source
Chemical Abundances in SFG and DLA
We investigate the chemical abundances of local star-forming galaxies which cause Damped Lyman Alpha lines. A metallicity versus redshift diagram is constructed, on which the chemical abundances of low-redshift star-forming galaxy populations are compared with those of high-redshift Damped Lyman Alpha systems.
Schulte-Ladbeck, Regina E. +2 more
openaire +2 more sources
Chemical abundances from planetary nebulae in local spiral galaxies
While the chemical abundances observed in bright planetary nebulae in local spiral galaxies are less varied than their counterparts in dwarfs, they provide new insight.
Marshall L. McCall, Michael G. Richer
core +1 more source
Stellar chemical abundances: In pursuit of the highest achievable precision [PDF]
The achievable level of precision on photospheric abundances of stars is a major limiting factor on investigations of exoplanet host star characteristics, the chemical histories of star clusters, and the evolution of the Milky Way and other galaxies ...
Bedell, Megan +5 more
core +1 more source
Cytarabine is a key therapy for acute myeloid leukaemia (AML), but its efficacy is limited by the dNTPase SAMHD1, which hydrolyses its active metabolite. Screening nucleotide biosynthesis inhibitors revealed that IMPDH inhibitors selectively sensitise SAMHD1‐proficient AML cells to cytarabine.
Miriam Yagüe‐Capilla +9 more
wiley +1 more source
Chemical abundances of hot post-AGB stars
Context. Hot post-AGB stars are luminous objects of low- and intermediate mass (0.8–8 M⊙) in the final stage of evolution, moving between the asymptotic giant branch (AGB) stars and planetary nebulae.
S. Daflon +3 more
core +1 more source
ASPCAP: THE APOGEE STELLAR PARAMETER AND CHEMICAL ABUNDANCES PIPELINE [PDF]
The Apache Point Observatory Galactic Evolution Experiment (APOGEE) has built the largest moderately highresolution (R≈22,500) spectroscopic map of the stars across the Milky Way, and including dust-obscured areas.
Cunha, Katia +62 more
core +1 more source

