Results 91 to 100 of about 55,137 (312)
Dimethyl fumarate (DMF) reduces growth of HPV‐positive cervical cancer spheroids and induces ferroptosis in cervical cancer cells via blocking SLC7A11/Glutathione (GSH) axis. Combination of subcytotoxic doses of DMF and cisplatin (CDDP) further suppresses spheroid growth and drives cell death in 2D culture models.
Carolina Punziano +6 more
wiley +1 more source
White dwarf–main-sequence (WD–MS) binary systems are essential probes for understanding binary stellar evolution and play a pivotal role in constraining theoretical models of various transient phenomena.
Jiadong Li +7 more
doaj +1 more source
The origin of the extreme hydrogen deficiency observed in the R Coronae Borealis (RCrB) stars remains poorly understood. A likely mechanism for producing this deficiency is one whereby the original hydrogen envelope of the star is engulfed and ...
Malaney, Robert A.
core
Life Cycle of a Low Mass Stars
In the present work, I shall explain the gravity mechanism and life cycle of a low mass Stars. For this purpose, some mathematical equations, and MATLAB Program could be used to draw the shape of a gravity as a dark fabric distortion in three dimensions ...
Sadiq, Sabir
core
The birthline for low-mass stars
Using the results of protostar theory, the locus in the Hertzsprung-Russell diagram is found where pre-main-sequence stars of subsolar mass should begin their quasi-static contraction phase and first appear as visible objects. This 'birthline' is in striking agreement with observations of T Tauri stars, providing a strong confirmation of the fact that ...
openaire +1 more source
Tumors contain diverse cellular states whose behavior is shaped by context‐dependent gene coordination. By comparing gene–gene relationships across biological contexts, we identify adaptive transcriptional modules that reorganize into distinct vulnerability axes.
Brian Nelson +9 more
wiley +1 more source
TOI-3288 b and TOI-4666 b: Two gas giants transiting low-mass stars characterised by NIRPS
Context. Gas giant planets orbiting low-mass stars (Teff ≲ 4600 K) are uncommon outcomes of planet formation. Increasing the sample of well-characterised giants around early M dwarfs will enable population-level studies of their properties, offering ...
Frensch Yolanda G. C. +68 more
doaj +1 more source
SMA and CARMA observations of young brown dwarfs in ρ Ophiuchi and Taurus
Molecular outflows provide vital information about the earliest stages in the birth of stars, studying the molecular outflow properties is therefore crucial for understanding how stars form.
Lee C.-F., Ngoc P.-B., Ho P.
doaj +1 more source
The accretion/ejection paradigm of low mass stars tested with HST
Low-mass stars and brown dwarfs: IMF, accretion and activity ,Volterra, Italy, 17-20 October 2004In the last few years new investigation techniques have allowed us to study in depth the spectacular phenomenon of protostellar jets, and to test the ...
Coffey, Deirdre +4 more
core
New theoretical yields of intermediate mass stars [PDF]
We present theoretical yields of H, 4He, 12C, 13C, 14N, and 16O for stars with initial masses between 0.8 and 8 $M_{\odot}$ and initial metallicities $Z = 0.001$, 0.004, 0.008, 0.02, and 0.04. We use the evolutionary tracks of the Geneva group up to the
M. A.T. Groenewegen +3 more
core +1 more source

