Catálogo de publicaciones - revistas
Science
Resumen/Descripción – provisto por la editorial
No disponible.
Palabras clave – provistas por la editorial
No disponibles.
Disponibilidad
| Institución detectada | Período | Navegá | Descargá | Solicitá |
|---|---|---|---|---|
| No detectada | desde mar. 1997 / hasta dic. 2023 | Science Journals |
Información
Tipo de recurso:
revistas
ISSN impreso
0036-8075
ISSN electrónico
1095-9203
Editor responsable
American Association for the Advancement of Science (AAAS)
País de edición
Estados Unidos
Fecha de publicación
1880-
Cobertura temática
Tabla de contenidos
Editors' Choice
Caroline Ash; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 242-243
Pathogens at the limits
Caroline Ash; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 242.1-243
A lanthanide secret handshake
Caroline Ash; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 242.2-242
Understanding preeclampsia
Caroline Ash; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 242.3-242
Dynamics of repulsive Fermi gases
Caroline Ash; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 242.4-243
Precision CRISPR editing
Caroline Ash; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 242.5-243
Targeting CH2 sites
Caroline Ash; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 242.6-243
Addressing a hairy problem
Caroline Ash; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 242.7-243
Luminescence and reactivity of a charge-transfer excited iron complex with nanosecond lifetime
Kasper Skov Kjær
; Nidhi Kaul
; Om Prakash
; Pavel Chábera
; Nils W. Rosemann
; Alireza Honarfar
; Olga Gordivska; Lisa A. Fredin
; Karl-Erik Bergquist; Lennart Häggström; Tore Ericsson; Linnea Lindh
; Arkady Yartsev
; Stenbjörn Styring
; Ping Huang; Jens Uhlig
; Jesper Bendix
; Daniel Strand
; Villy Sundström
; Petter Persson
; Reiner Lomoth
; Kenneth Wärnmark
<jats:title>Orange-glowing iron at room temperature</jats:title> <jats:p> Many photoactive coordination compounds contain precious metals. Replacing ruthenium with more–earth-abundant iron has been a long-sought goal, but iron compounds generally relax too rapidly after light absorption to channel the energy productively. Kjær <jats:italic>et al.</jats:italic> prepared an iron compound with an excited state stable enough to emit light for nanoseconds, or that could engage in bimolecular electron transfer (see the Perspective by Young and Oldacre). Targeting a ligand-to-metal rather than metal-to-ligand charge-transfer state was key to the achievement, as was the octahedral coordination environment rigidly enforced by two tridentate carbene ligands. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6424" page="249" related-article-type="in-this-issue" vol="363" xlink:href="10.1126/science.aau7160">249</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6424" page="225" related-article-type="in-this-issue" vol="363" xlink:href="10.1126/science.aav9866">225</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. 249-253
Earth and Moon impact flux increased at the end of the Paleozoic
Sara Mazrouei
; Rebecca R. Ghent
; William F. Bottke
; Alex H. Parker; Thomas M. Gernon
<jats:title>Impact rates on Earth and the Moon</jats:title> <jats:p> The rate at which impacts produce craters on the Moon is used to calibrate ages in planetary science. Earth should also have received similar numbers of impacts, but many craters have been hidden by erosion, ice sheets, and so on. Mazrouei <jats:italic>et al.</jats:italic> used infrared images of the Moon to estimate the ages of young lunar craters (see the Perspective by Koeberl). They found that the impact rate increased within the past ∼500 million years, a conclusion strengthened by an analysis of known impact craters on Earth. Crater size distributions are the same on Earth and the Moon over this period, implying that terrestrial erosion affects all craters equally, regardless of their size. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6424" page="253" related-article-type="in-this-issue" vol="363" xlink:href="10.1126/science.aar4058">253</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6424" page="224" related-article-type="in-this-issue" vol="363" xlink:href="10.1126/science.aav8480">224</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. 253-257