Results 61 to 70 of about 1,100,727 (344)

Mapping the evolution of mitochondrial complex I through structural variation

FEBS Letters, EarlyView.
Respiratory complex I (CI) is crucial for bioenergetic metabolism in many prokaryotes and eukaryotes. It is composed of a conserved set of core subunits and additional accessory subunits that vary depending on the organism. Here, we categorize CI subunits from available structures to map the evolution of CI across eukaryotes. Respiratory complex I (CI)
Dong‐Woo Shin, Tingting Chen, James A. Letts   +2 more
wiley   +1 more source

Stellar Coronal and Wind Models: Impact on Exoplanets

, 2017
Surface magnetism is believed to be the main driver of coronal heating and stellar wind acceleration. Coronae are believed to be formed by plasma confined in closed magnetic coronal loops of the stars, with winds mainly originating in open magnetic field
A Maggio, A Morgenthaler, A Morgenthaler, A Reiners, A Reiners, A Reiners, A Strugarek, A Telleschi, A. Skumanich, AA Pevtsov, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA Vidotto, AA West, AF Lanza, B Holst van der, B Holst van der, B Zieger, BA Nicholson, BE Wood, BE Wood, BE Wood, BE Wood, BE Wood, BJ Wargelin, BO Demory, C Catala, C Garraffo, C Johnstone, C. P. Johnstone, CM Johns-Krull, CM Johns-Krull, CP Folsom, CP Johnstone, CP Johnstone, D Arzoumanian, D Bisikalo, D Buzasi, D Falceta-Gonçalves, D Lai, E Shkolnik, EF Guinan, EJ Gaidos, F Bagenal, G Anglada-Escudé, G Scandariato, GAJ Hussain, GAJ Hussain, GAJ Hussain, GHJ Oord van den, GW Pneuman, H Lammer, H Lammer, H Washimi, I Baraffe, I Pillitteri, I Ribas, I. Ribas, IA Waite, IA Waite, IA Waite, Ignasi Ribas, IV Sokolov, J Donati, J Donati, J Donati, J Donati, J Llama, J Morin, J Morin, J Morin, J Morin, J Sanz-Forcada, J Zendejas, Jackie Villadsen, JD Alvarado-Gómez, Jeremy Lim, JF Donati, JF Donati, JF Donati, JF Donati, JF Donati, JF Donati, JF Donati, JF Donati, JF Donati, JF Donati, JH Debes, JI Zuluaga, JJG Lima, JM Grießmeier, JM Grießmeier, JV Hollweg, K Tsinganos, KG Kislyakova, L Hartmann, L. Mestel, M Guedel, M Guedel, M Güdel, M Jardine, M Jardine, MG Sterenborg, ML Khodachenko, ML Khodachenko, N Pizzolato, NJ Wright, O Cohen, O Cohen, O. Cohen, O. Cohen, P Lang, P Petit, P Petit, P Testa, R Fares, R Fares, R Fares, R Fares, R Keppens, R Pallavicini, RD Jeffries, Robert P. Kraft, Rui F. Pinto, RVE Lovelace, S Boro Saikia, S Boro Saikia, S Matt, S. V. Jeffers, SC Marsden, SC Marsden, SG Parsons, SH Yang, SK Solanki, SL Li, SP Matt, SR Cranmer, SR Cranmer, T Matsakos, T Matsumoto, Takuma Matsumoto, TE Holzer, Theresa Lüftinger, TK Suzuki, V Jatenco-Pereira, V Réville, V See, V. Bourrier, V. Bourrier, WH Ip   +162 more
core   +1 more source

The Efficiency of Mass Accretion and Disc Structure from the Stellar Wind Mass Transfer in Binary Systems

Universe
There have been many research works involving mass transfer in stellar binaries, all of which are limited to certain systems with specific binary parameters.
Bushra Ata Ali, Hastyar Omar Mohammed, Peshwaz Abdulkareem Abdoul   +2 more
doaj   +1 more source

Thermal winds in stellar mass black hole and neutron star binary systems [PDF]

, 2016
Black hole binaries show equatorial disc winds at high luminosities, which apparently disappear during the spectral transition to the low/hard state. This is also where the radio jet appears, motivating speculation that both wind and jet are driven by ...
C. Done, R. Tomaru, Tad Takahashi Durham University, UK., Isasjaxa, T. University, Japan.   +6 more
semanticscholar   +1 more source

Plasmodium falciparum gametogenesis essential protein 1 (GEP1) is a transmission‐blocking target

FEBS Letters, EarlyView.
This study shows Plasmodium falciparum GEP1 is vital for activating sexual stages of malarial parasites even independently of a mosquito factor. Knockout parasites completely fail gamete formation even when a phosphodiesterase inhibitor is added. Two single‐nucleotide polymorphisms (V241L and S263P) are found in 12%–20% of field samples.
Frederik Huppertz, Milagros Siebeck Caturelli, Lina S. Lehmann, Florian Kurth, Alexander G. Maier, Kai Matuschewski   +5 more
wiley   +1 more source

Stellar magnetism, winds and their effects on planetary environments

, 2016
Here, I review some recent works on magnetism of cool, main-sequence stars, their winds and potential impact on surrounding exoplanets. The winds of these stars are very tenuous and persist during their lifetime.
Vidotto, A. A.
core   +1 more source

Galactic Centre stellar winds and Sgr A* accretion [PDF]

, 2005
(ABRIDGED) We present in detail our new 3D numerical models for the accretion of stellar winds on to Sgr A*. In our most sophisticated models, we put stars on realistic orbits around Sgr A*, include `slow' winds (300 km/s), and account for radiative ...
Cuadra, J., Di Matteo, T., Nayakshin, S., Springel, V.   +3 more
core   +2 more sources

Biophysical analysis of angiotensin II and amyloid‐β cross‐interaction in aggregation and membrane disruption

FEBS Letters, EarlyView.
Angiotensin II (AngII), a neuropeptide, interacts with amyloid‐β (Aβ), a key player in Alzheimer's disease. This study reveals that AngII reduces Aβ aggregation and membrane disruption in vitro. Biophysical assays and molecular modeling suggest AngII binds disordered Aβ forms, potentially modulating early amyloidogenic events and contributing to ...
Mohsen Habibnia, Eric Catalina‐Hernandez, Maialen Cabrerizo‐Idiazabal, Ramon Barnadas‐Rodríguez, Mario Lopez‐Martin, Alex Peralvarez‐Marin   +5 more
wiley   +1 more source

X-ray diagnostics of massive star winds

, 2016
Nearly all types of massive stars with radiatively driven stellar winds are X-ray sources that can be observed by the presently operating powerful X-ray telescopes.
Oskinova, Lidia
core   +1 more source

Modeling T Tauri Winds from He I 10830 Profiles [PDF]

, 2006
The high opacity of He I 10830 makes it an exceptionally sensitive probe of the inner wind geometry of accreting T Tauri stars. In this line blueshifted absorption below the continuum results from simple scattering of stellar photons, a situation which ...
Blandford R. D., Dougados C., John Kwan, Kurosawa R., Lavalley-Fouquet C., Suzan Edwards, William Fischer   +6 more
core   +3 more sources