Results 221 to 230 of about 26,707 (264)

Insights into early continental crust formation from the most ancient heart of Scotland. [PDF]

Nat Commun
Volante S, Torres-Mancinelli F, Kaempf J, Barrote V, Johnson T, Kirkland C, Scicchitano MR, Tavazzani L, Basak S, Bouvier AS, Dziggel A, Gerdes A.   +11 more
europepmc   +1 more source

Strongest constraint on the parastatistical Quon model with the VIP-2 measurements. [PDF]

Sci Rep
Porcelli A, Piscicchia K, Bazzi M, Bortolotti N, Bragadireanu M, Cargnelli M, Clozza A, Paolis L, Del Grande R, Guaraldo C, Iliescu M, Laubenstein M, Manti S, Marton J, Napolitano F, Scordo A, Sgaramella F, Sirghi DL, Sirghi F, Zmeskal J, Curceanu C.   +20 more
europepmc   +1 more source

Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]

Space Sci Rev
Szalay JR, Provornikova E, Ayari E, Bzowski M, Christian ER, Funsten HO, Galli A, Gkioulidou M, Horányi M, Livi S, McComas DJ, Möbius E, Ogasawara K, Rahmanifard F, Rankin JS, Reisenfeld DB, Schwadron NA, Sternovsky Z, Swaczyna P, Turner D, Zank GP, Zirnstein EJ.   +21 more
europepmc   +1 more source

A nearby dark molecular cloud in the Local Bubble revealed via H₂ fluorescence. [PDF]

Nat Astron
Burkhart B, Dharmawardena TE, Bialy S, Haworth TJ, Cruz Aguirre F, Jo YS, Andersson BG, Chung H, Edelstein J, Grenier I, Hamden ET, Han W, Hoadley K, Lee MY, Min KW, Müller T, Pattle K, Peek JEG, Pleiss G, Schiminovich D, Seon KI, Wilson AG, Zucker C.   +22 more
europepmc   +1 more source

Nucleation of α-pinene oxidation products with sulfuric acid.

Environ Sci Atmos
Sommer E, Almeida J, Yu W, Simon M, Möller F, Xenofontos C, Pozzer A, Zheng Z, Bhattacharyya N, Alfaouri D, Atabakhsh S, Baalbaki R, Beckmann H, Berntheusel M, Bogert P, Busato M, Canagaratna M, Caudillo-Plath L, Chassaing A, Cruz-Simbron R, Dada L, DeVivo J, Duplissy J, Gordon H, Granzin M, Schute LG, Hartl HG, Hirvensalo E, Jacobshagen A, Judmaier B, Sebastian MK, Klebach H, Koemets P, Kohl M, Konrat R, Krüger T, Kunkler F, Kürten A, Leiminger M, Lietzke CJ, Liu L, Mauldin R, Mentler B, Morawiec A, Müller M, Petäjä T, Pignatelli A, Rato P, Reinecke T, Richter S, Rörup B, Ruhl S, Russell DM, Scholz W, Shen J, Stinchfield A, Thakur RC, Tong Y, Top J, Umo NS, Weissbacher J, Yang B, Zauner-Wieczorek M, Zhang J, Amorim A, Baltensberger U, Christoudias T, Curtius J, Donahue NM, El Haddad I, Flagan RC, Hansel A, Harder H, He XC, Junninen H, Kulmala M, Lehtipalo K, Lelieveld J, Möhler O, Schobesberger S, Tomé A, Volkamer R, Worsnop DR, Onnela A, Winkler PM, Kirkby J.   +85 more
europepmc   +1 more source

Paper-based lead-free thin film X-ray detectors with high sensitivity and superior environmental stability

Zhao Q, Liu Y, Chen Y, Gong W, Li X, Zhou B, Huang H, Han N, Chen S, Zhang B, Li J, Castellanos-Gomez A, Gnatyuk V, Nan W, Wang T.   +14 more
europepmc   +1 more source

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Viewing the sun as an X-ray star

Advances in Space Research, 2003
Abstract The Sun is the late-type star we can study with the highest level of detail. In the interpretation of stellar data, therefore, it is often assumed that the physical processes of the coronae of late-type stars are similar to those of the solar corona, i.e. the “solar-stellar analogy”.
Orlando, S., PERES, Giovanni, REALE, Fabio   +2 more
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X–rays from stars

Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences, 2002
More than two years of observation with Chandra and XMM-Newton has provided a rich harvest of new results on the physics of stellar coronae and winds. High-resolution X-ray spectroscopy in particular has opened new windows to the structure, the dynamics and the composition of stellar atmospheres.
openaire   +3 more sources

X-Ray Binaries with Be Stars

Astronomy Reports
The basic properties of Be stars and X-ray binary systems containing these stars are considered. In the vast majority of these systems the Be stars' companions are neutron stars accreting matter from the decretion disk of a rapidly rotating Be star. The observed properties of such systems are studied within the framework of the hypothesis that
A. V. Fedorova, A. V. Tutukov
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X Rays in the Stars

The British Journal of Radiology, 1930
There is a celebrated toast, “Here's to Pure Mathematics! And may they never be of any use to anybody!” It is a pious wish which has small hope of ever being fulfilled. However high-mindedly the devotee may strive to follow knowledge for its own sake uninfluenced by motives of practical utility his results have a way of turning out to be useful in ...
openaire   +1 more source