Results 241 to 250 of about 65,066 (300)
Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Living Rev Sol PhysVeronig AM, Dissauer K, Kliem B, Downs C, Hudson HS, Jin M, Osten R, Podladchikova T, Prasad A, Qiu J, Thompson B, Tian H, Vourlidas A. +12 moreeuropepmc +1 more sourceThe Renal Activity Index for Lupus Identifies Active Renal Disease and Treatment Response in Adult Patients With Systemic Lupus Erythematosus and Lupus Nephritis
Arthritis Care &Research, EarlyView.Objective
We evaluated the ability of the Renal Activity Index for Lupus (RAIL) to discriminate active lupus nephritis (LN) in adult patients with active systemic lupus erythematosus (SLE) and differentiate LN treatment response. Methods
Urine samples from adults with biopsy‐proven active class III and IV LN from TULIP‐LN (active LN group ...Hermine I. Brunner, Ellen M. Cody, Prasad Devarajan, Bin Huang, Chen Chen, Dominic Sinibaldi, Madhu Ramaswamy, Jacob Knagenhjelm, Frederick Jones, Philip Z. Brohawn, Raj Tummala, Catharina Lindholm, Wendy I. White +12 morewiley +1 more sourceMultiple outflows and delayed ejections revealed by early imaging of novae. [PDF]
Nat AstronAydi E, Monnier JD, Mérand A, Schaefer GH, Chomiuk L, Otulakowska-Hypka M, Fan JL, Li KL, Sokolovsky KV, Salinas R, Tucker M, Shappee B, Rudy R, Page KL, Kuin NPM, Buckley DAH, Craig P, Izzo L, Linford J, Metzger BD, Mukai K, Orio M, Shen KJ, Strader J, Sokoloski JL, Williams RE, Williams MN, Habtie GR, Kraus S, Anugu N, Bouquin JL, Chhabra S, Codron I, Gardner T, Gutierrez M, Ibrahim N, Lanthermann C, Setterholm BR, Ashall C, Hinkle JT, Jaeger T, Payne AV. +41 moreeuropepmc +1 more sourceNeutron capture measurements for s-process nucleosynthesis: A review about CERN n_TOF developments and contributions. [PDF]
Eur Phys J A Hadron NuclDomingo-Pardo C, Aberle O, Alcayne V, Alpar G, Halabi MA, Amaducci S, Babiano V, Bacak M, Balibrea-Correa J, Bartolomé J, Bernardes AP, Gameiro BB, Berthoumieux E, Beyer R, Birch M, Boromiza M, Bosnar D, Brusasco B, Caamaño M, Cahuzac A, Calviño F, Calviani M, Cano-Ott D, Casanovas A, Castelluccio DM, Catlett D, Cerutti F, Cescutti G, Chiaveri E, Claps G, Colombetti P, Colonna N, Camprini PC, Cortés G, Cortés-Giraldo MA, Cosentino L, Cristallo S, D'Ottavi A, de la Fuente Rosales G, Dellmann SF, Diakaki M, Di Castro M, Di Chicco A, Dietz M, Dupont E, Durán I, Eleme Z, Eslami M, Fargier S, Fernández-Domínguez B, Finocchiaro P, Flanagan W, Furman V, Gandhi A, García-Infantes F, Gawlik-Ramiega A, Gervino G, Gilardoni S, González-Romero E, Goula S, Griesmayer E, Guerrero C, Gunsing F, Gustavino C, Heyse J, Hillman W, Jenkins DG, Jericha E, Junghans A, Kadi Y, Kaperoni K, Kelly I, Kokkoris M, Kopatch Y, Krtička M, Kyritsis N, Lederer-Woods C, Lerendegui-Marco J, Manna A, Martínez T, Martínez-Cañada M, Masi A, Massimi C, Mastinu P, Mastromarco M, Maugeri EA, Mazzone A, Mendoza E, Mengoni A, Michalopoulou V, Milazzo PM, Moldenhauer J, Mucciola R, González EM, Musumarra A, Negret A, Odusina E, Papanikolaou D, Patronis N, Pavón-Rodríguez JA, Pellegriti MG, Pérez-Maroto P, de Rada Fiol AP, Perfetto G, Perkowski J, Petrone C, Pieretti N, Piersanti L, Pirovano E, Porras I, Praena J, Quesada JM, Reifarth R, Rochman D, Romanets Y, Rooney A, Rovira G, Rubbia C, Sánchez-Caballero A, Sahoo RN, Scarpa D, Schillebeeckx P, Smith AG, Sosnin NV, Spelta M, Stamati ME, Stasiak K, Tagliente G, Tarifeño-Saldivia A, Tarrío D, Torres-Sánchez P, Tosi S, Tsiledakis G, Valenta S, Vaz P, Vecchio G, Vescovi D, Vlachoudis V, Vlastou R, Wallner A, Weiss C, Woods PJ, Wright T, Wu R, Žugec P, The n_TOF Collaboration. +145 moreeuropepmc +1 more sourceThe dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant
Munoz-Sanchez G, Kalitsounaki M, de Wit S, Antoniadis K, Bonanos A, Zapartas E, Boutsia K, Christodoulou E, Maravelias G, Soszyński I, Udalski A. +10 moreeuropepmc +1 more sourceAn Abrupt Change in the Disk Fraction of Free-Floating Planets at the Deuterium-Burning Ignition Limit
Rodrigues T, Bouy H, Raymond S, Martín E, Bertin E, Romero JO, Barrado D, Huélamo N, Tamura M, Roig NM, Galli P, Cuillandre J. +11 moreeuropepmc +1 more sourceSome of the next articles are maybe not open access.Related searches:
Strong Stellar Winds
Science, 1980 The hottest and most luminous stars lose a substantial fraction of their mass in strong stellar winds. These winds not only affect the evolution of the star, they also carve huge expanding cavities in the surrounding interstellar medium, possibly affecting star formation. The winds are probably driven by radiation pressure, but uncertainties persist in P S, Conti, R, McCrayopenaire +4 more sources