Results 51 to 60 of about 3,488,609 (297)

Prospecting the protein design landscape

open access: yesFEBS Letters, EarlyView.
This review outlines the current state of various protein design approaches. We discuss the current possibilities enabled by recently released tools, highlight future avenues to pursue in protein design, and underscore the crucial role of key databases and resources for successful protein design workflows.
Jakob R. Riccabona   +4 more
wiley   +1 more source

Effects of strong magnetic fields in dense stellar matter [PDF]

open access: yes, 2013
We study the effects of strong magnetic fields in dense stellar matter within an effective relativistic equation of state with the inclusion of hyperons and Δ(1232)-isobar degrees of freedom.
LAVAGNO, Andrea, LINGUA, FABIO
core   +2 more sources

Smaller is better: nanobodies meet NMR

open access: yesFEBS Letters, EarlyView.
Nanobodies are single‐domain antigen‐binding fragments derived from camelid heavy chain antibodies. Their small size, high stability, and exceptional specificity make nanobodies uniquely useful probes for NMR studies of protein dynamics, transient conformational states, and protein–protein interactions.
Oleg Y. Dmitriev
wiley   +1 more source

Simplified Model of the Solar Magnetic Field

open access: yesThe Astrophysical Journal
This paper considers a structure consisting of two rings of magnetic dipoles symmetrical relative to the equatorial plane as a possible model for the source of the solar magnetic field.
Igor G. Kosakovskij
doaj   +1 more source

The rotation–magnetism relationship in solar-type stars

open access: yesAstronomy & Astrophysics
Context. The rotation–activity relationship of G-type stars results from surface magnetic fields emerging from the interior. How the magnetic flux and its emergence rate scale with rotation rate are not well understood, both observationally and ...
Işık Emre   +3 more
doaj   +1 more source

Updating the Dartmouth stellar evolution model grid: Pre-main-sequence models & magnetic fields [PDF]

open access: yes, 2014
Poster from The 18th Workshop on Cool Stars, Stellar Systems, and the Sun on updating the Dartmouth stellar evolution model grid. Additions include models of pre-main-sequence stars, magnetic fields, deuterium burning, and a revised treatment of surface ...
Chaboyer, Brian   +5 more
core   +1 more source

Unlocking the potential of cell‐permeable nanobodies for intracellular applications

open access: yesFEBS Letters, EarlyView.
This review outlines current strategies for delivery of nanobodies into cells and highlights recent examples of functional applications. By addressing and manipulating intracellular targets, these molecules hold great potential for treating cancer, respiratory diseases and neurological disorders, making this a vibrant area of research in the biomedical
Mariona Gené‐Verdés   +2 more
wiley   +1 more source

Magnetic Fields in M-dwarf Members of the Pleiades Open Cluster Using APOGEE Spectra

open access: yesThe Astrophysical Journal
Average magnetic field measurements are presented for 62 M-dwarf members of the Pleiades open cluster, derived from Zeeman-enhanced Fe i lines in the H band.
Fábio Wanderley   +12 more
doaj   +1 more source

Flow Enabled Target Capture Halbach‐based magnetic enrichment increases circulating tumor cell capture from blood in metastatic cancer patients

open access: yesMolecular Oncology, EarlyView.
Pair‐wise comparison of the CellSearch and FETCH enrichment technologies for circulating tumor cells (CTCs) from metastatic breast, prostate, and small cell lung cancer patients shows an increased capture of CTCs using FETCH enrichment. The clinical implementation of circulating tumor cells (CTCs) as a predictive tool for therapy efficacy in the ...
Michiel Stevens   +6 more
wiley   +1 more source

Stellar dynamics: Rotation, convection, and magnetic fields [PDF]

open access: yes, 2015
Stars are changing entities in a constant evolution during their lives. At non-secular time scales (from seconds to years) the effect of dynamical processes such as convection, rotation, and magnetic fields can modify the stellar oscillations. Convection excites acoustic modes in solar-like stars, while rotation and magnetic fields can perturb the ...
Mathur, S., Ballot, J., Garcia, R. A.
openaire   +2 more sources

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