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
Posture and waggle control butterfly flight
Patrick Monahan
Palabras clave: Multidisciplinary.
Pp. No disponible
The small satellites of Pluto as observed by New Horizons
H. A. Weaver; M. W. Buie; B. J. Buratti; W. M. Grundy; T. R. Lauer; C. B. Olkin; A. H. Parker; S. B. Porter; M. R. Showalter; J. R. Spencer; S. A. Stern; A. J. Verbiscer; W. B. McKinnon; J. M. Moore; S. J. Robbins; P. Schenk; K. N. Singer; O. S. Barnouin; A. F. Cheng; C. M. Ernst; C. M. Lisse; D. E. Jennings; A. W. Lunsford; D. C. Reuter; D. P. Hamilton; D. E. Kaufmann; K. Ennico; L. A. Young; R. A. Beyer; R. P. Binzel; V. J. Bray; A. L. Chaikin; J. C. Cook; D. P. Cruikshank; C. M. Dalle Ore; A. M. Earle; G. R. Gladstone; C. J. A. Howett; I. R. Linscott; F. Nimmo; J. Wm. Parker; S. Philippe; S. Protopapa; H. J. Reitsema; B. Schmitt; T. Stryk; M. E. Summers; C. C. C. Tsang; H. H. B. Throop; O. L. White; A. M. Zangari
<jats:title>New Horizons unveils the Pluto system</jats:title> <jats:p> In July 2015, the New Horizons spacecraft flew through the Pluto system at high speed, humanity's first close look at this enigmatic system on the outskirts of our solar system. In a series of papers, the New Horizons team present their analysis of the encounter data downloaded so far: Moore <jats:italic>et al.</jats:italic> present the complex surface features and geology of Pluto and its large moon Charon, including evidence of tectonics, glacial flow, and possible cryovolcanoes. Grundy <jats:italic>et al.</jats:italic> analyzed the colors and chemical compositions of their surfaces, with ices of H <jats:sub>2</jats:sub> O, CH <jats:sub>4</jats:sub> , CO, N <jats:sub>2</jats:sub> , and NH <jats:sub>3</jats:sub> and a reddish material which may be tholins. Gladstone <jats:italic>et al.</jats:italic> investigated the atmosphere of Pluto, which is colder and more compact than expected and hosts numerous extensive layers of haze. Weaver <jats:italic>et al.</jats:italic> examined the small moons Styx, Nix, Kerberos, and Hydra, which are irregularly shaped, fast-rotating, and have bright surfaces. Bagenal <jats:italic>et al.</jats:italic> report how Pluto modifies its space environment, including interactions with the solar wind and a lack of dust in the system. Together, these findings massively increase our understanding of the bodies in the outer solar system. They will underpin the analysis of New Horizons data, which will continue for years to come. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue pp. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6279" page="1284" related-article-type="in-this-issue" vol="351" xlink:href="10.1126/science.aad7055">1284</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad9189">10.1126/science.aad9189</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad8866">10.1126/science.aad8866</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aae0030">10.1126/science.aae0030</jats:related-article> , & <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad9045">10.1126/science.aad9045</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. No disponible
The atmosphere of Pluto as observed by New Horizons
G. Randall Gladstone; S. Alan Stern; Kimberly Ennico; Catherine B. Olkin; Harold A. Weaver; Leslie A. Young; Michael E. Summers; Darrell F. Strobel; David P. Hinson; Joshua A. Kammer; Alex H. Parker; Andrew J. Steffl; Ivan R. Linscott; Joel Wm. Parker; Andrew F. Cheng; David C. Slater; Maarten H. Versteeg; Thomas K. Greathouse; Kurt D. Retherford; Henry Throop; Nathaniel J. Cunningham; William W. Woods; Kelsi N. Singer; Constantine C. C. Tsang; Eric Schindhelm; Carey M. Lisse; Michael L. Wong; Yuk L. Yung; Xun Zhu; Werner Curdt; Panayotis Lavvas; Eliot F. Young; G. Leonard Tyler; F. Bagenal; W. M. Grundy; W. B. McKinnon; J. M. Moore; J. R. Spencer; T. Andert; J. Andrews; M. Banks; B. Bauer; J. Bauman; O. S. Barnouin; P. Bedini; K. Beisser; R. A. Beyer; S. Bhaskaran; R. P. Binzel; E. Birath; M. Bird; D. J. Bogan; A. Bowman; V. J. Bray; M. Brozovic; C. Bryan; M. R. Buckley; M. W. Buie; B. J. Buratti; S. S. Bushman; A. Calloway; B. Carcich; S. Conard; C. A. Conrad; J. C. Cook; D. P. Cruikshank; O. S. Custodio; C. M. Dalle Ore; C. Deboy; Z. J. B. Dischner; P. Dumont; A. M. Earle; H. A. Elliott; J. Ercol; C. M. Ernst; T. Finley; S. H. Flanigan; G. Fountain; M. J. Freeze; J. L. Green; Y. Guo; M. Hahn; D. P. Hamilton; S. A. Hamilton; J. Hanley; A. Harch; H. M. Hart; C. B. Hersman; A. Hill; M. E. Hill; M. E. Holdridge; M. Horanyi; A. D. Howard; C. J. A. Howett; C. Jackman; R. A. Jacobson; D. E. Jennings; H. K. Kang; D. E. Kaufmann; P. Kollmann; S. M. Krimigis; D. Kusnierkiewicz; T. R. Lauer; J. E. Lee; K. L. Lindstrom; A. W. Lunsford; V. A. Mallder; N. Martin; D. J. McComas; R. L. McNutt; D. Mehoke; T. Mehoke; E. D. Melin; M. Mutchler; D. Nelson; F. Nimmo; J. I. Nunez; A. Ocampo; W. M. Owen; M. Paetzold; B. Page; F. Pelletier; J. Peterson; N. Pinkine; M. Piquette; S. B. Porter; S. Protopapa; J. Redfern; H. J. Reitsema; D. C. Reuter; J. H. Roberts; S. J. Robbins; G. Rogers; D. Rose; K. Runyon; M. G. Ryschkewitsch; P. Schenk; B. Sepan; M. R. Showalter; M. Soluri; D. Stanbridge; T. Stryk; J. R. Szalay; M. Tapley; A. Taylor; H. Taylor; O. M. Umurhan; A. J. Verbiscer; M. H. Versteeg; M. Vincent; R. Webbert; S. Weidner; G. E. Weigle; O. L. White; K. Whittenburg; B. G. Williams; K. Williams; S. Williams; A. M. Zangari; E. Zirnstein;
<jats:title>New Horizons unveils the Pluto system</jats:title> <jats:p> In July 2015, the New Horizons spacecraft flew through the Pluto system at high speed, humanity's first close look at this enigmatic system on the outskirts of our solar system. In a series of papers, the New Horizons team present their analysis of the encounter data downloaded so far: Moore <jats:italic>et al.</jats:italic> present the complex surface features and geology of Pluto and its large moon Charon, including evidence of tectonics, glacial flow, and possible cryovolcanoes. Grundy <jats:italic>et al.</jats:italic> analyzed the colors and chemical compositions of their surfaces, with ices of H <jats:sub>2</jats:sub> O, CH <jats:sub>4</jats:sub> , CO, N <jats:sub>2</jats:sub> , and NH <jats:sub>3</jats:sub> and a reddish material which may be tholins. Gladstone <jats:italic>et al.</jats:italic> investigated the atmosphere of Pluto, which is colder and more compact than expected and hosts numerous extensive layers of haze. Weaver <jats:italic>et al.</jats:italic> examined the small moons Styx, Nix, Kerberos, and Hydra, which are irregularly shaped, fast-rotating, and have bright surfaces. Bagenal <jats:italic>et al.</jats:italic> report how Pluto modifies its space environment, including interactions with the solar wind and a lack of dust in the system. Together, these findings massively increase our understanding of the bodies in the outer solar system. They will underpin the analysis of New Horizons data, which will continue for years to come. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue pp. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6279" page="1284" related-article-type="in-this-issue" vol="351" xlink:href="10.1126/science.aad7055">1284</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad9189">10.1126/science.aad9189</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad8866">10.1126/science.aad8866</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aae0030">10.1126/science.aae0030</jats:related-article> , & <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad9045">10.1126/science.aad9045</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. No disponible
Pluto’s interaction with its space environment: Solar wind, energetic particles, and dust
F. Bagenal; M. Horányi; D. J. McComas; R. L. McNutt; H. A. Elliott; M. E. Hill; L. E. Brown; P. A. Delamere; P. Kollmann; S. M. Krimigis; M. Kusterer; C. M. Lisse; D. G. Mitchell; M. Piquette; A. R. Poppe; D. F. Strobel; J. R. Szalay; P. Valek; J. Vandegriff; S. Weidner; E. J. Zirnstein; S. A. Stern; K. Ennico; C. B. Olkin; H. A. Weaver; L. A. Young; G. R. Gladstone; W. M. Grundy; W. B. McKinnon; J. M. Moore; J. R. Spencer; T. Andert; J. Andrews; M. Banks; B. Bauer; J. Bauman; O. S. Barnouin; P. Bedini; K. Beisser; R. A. Beyer; S. Bhaskaran; R. P. Binzel; E. Birath; M. Bird; D. J. Bogan; A. Bowman; V. J. Bray; M. Brozovic; C. Bryan; M. R. Buckley; M. W. Buie; B. J. Buratti; S. S. Bushman; A. Calloway; B. Carcich; A. F. Cheng; S. Conard; C. A. Conrad; J. C. Cook; D. P. Cruikshank; O. S. Custodio; C. M. Dalle Ore; C. Deboy; Z. J. B. Dischner; P. Dumont; A. M. Earle; J. Ercol; C. M. Ernst; T. Finley; S. H. Flanigan; G. Fountain; M. J. Freeze; T. Greathouse; J. L. Green; Y. Guo; M. Hahn; D. P. Hamilton; S. A. Hamilton; J. Hanley; A. Harch; H. M. Hart; C. B. Hersman; A. Hill; D. P. Hinson; M. E. Holdridge; A. D. Howard; C. J. A. Howett; C. Jackman; R. A. Jacobson; D. E. Jennings; J. A. Kammer; H. K. Kang; D. E. Kaufmann; D. Kusnierkiewicz; T. R. Lauer; J. E. Lee; K. L. Lindstrom; I. R. Linscott; A. W. Lunsford; V. A. Mallder; N. Martin; D. Mehoke; T. Mehoke; E. D. Melin; M. Mutchler; D. Nelson; F. Nimmo; J. I. Nunez; A. Ocampo; W. M. Owen; M. Paetzold; B. Page; A. H. Parker; J. W. Parker; F. Pelletier; J. Peterson; N. Pinkine; S. B. Porter; S. Protopapa; J. Redfern; H. J. Reitsema; D. C. Reuter; J. H. Roberts; S. J. Robbins; G. Rogers; D. Rose; K. Runyon; K. D. Retherford; M. G. Ryschkewitsch; P. Schenk; E. Schindhelm; B. Sepan; M. R. Showalter; K. N. Singer; M. Soluri; D. Stanbridge; A. J. Steffl; T. Stryk; M. E. Summers; M. Tapley; A. Taylor; H. Taylor; H. B. Throop; C. C. C. Tsang; G. L. Tyler; O. M. Umurhan; A. J. Verbiscer; M. H. Versteeg; M. Vincent; R. Webbert; G. E. Weigle; O. L. White; K. Whittenburg; B. G. Williams; K. Williams; S. Williams; W. W. Woods; A. M. Zangari;
<jats:title>New Horizons unveils the Pluto system</jats:title> <jats:p> In July 2015, the New Horizons spacecraft flew through the Pluto system at high speed, humanity's first close look at this enigmatic system on the outskirts of our solar system. In a series of papers, the New Horizons team present their analysis of the encounter data downloaded so far: Moore <jats:italic>et al.</jats:italic> present the complex surface features and geology of Pluto and its large moon Charon, including evidence of tectonics, glacial flow, and possible cryovolcanoes. Grundy <jats:italic>et al.</jats:italic> analyzed the colors and chemical compositions of their surfaces, with ices of H <jats:sub>2</jats:sub> O, CH <jats:sub>4</jats:sub> , CO, N <jats:sub>2</jats:sub> , and NH <jats:sub>3</jats:sub> and a reddish material which may be tholins. Gladstone <jats:italic>et al.</jats:italic> investigated the atmosphere of Pluto, which is colder and more compact than expected and hosts numerous extensive layers of haze. Weaver <jats:italic>et al.</jats:italic> examined the small moons Styx, Nix, Kerberos, and Hydra, which are irregularly shaped, fast-rotating, and have bright surfaces. Bagenal <jats:italic>et al.</jats:italic> report how Pluto modifies its space environment, including interactions with the solar wind and a lack of dust in the system. Together, these findings massively increase our understanding of the bodies in the outer solar system. They will underpin the analysis of New Horizons data, which will continue for years to come. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue pp. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6279" page="1284" related-article-type="in-this-issue" vol="351" xlink:href="10.1126/science.aad7055">1284</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad9189">10.1126/science.aad9189</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad8866">10.1126/science.aad8866</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aae0030">10.1126/science.aae0030</jats:related-article> , & <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad9045">10.1126/science.aad9045</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. No disponible
Surface compositions across Pluto and Charon
W. M. Grundy; R. P. Binzel; B. J. Buratti; J. C. Cook; D. P. Cruikshank; C. M. Dalle Ore; A. M. Earle; K. Ennico; C. J. A. Howett; A. W. Lunsford; C. B. Olkin; A. H. Parker; S. Philippe; S. Protopapa; E. Quirico; D. C. Reuter; B. Schmitt; K. N. Singer; A. J. Verbiscer; R. A. Beyer; M. W. Buie; A. F. Cheng; D. E. Jennings; I. R. Linscott; J. Wm. Parker; P. M. Schenk; J. R. Spencer; J. A. Stansberry; S. A. Stern; H. B. Throop; C. C. C. Tsang; H. A. Weaver; G. E. Weigle; L. A. Young;
<jats:title>New Horizons unveils the Pluto system</jats:title> <jats:p> In July 2015, the New Horizons spacecraft flew through the Pluto system at high speed, humanity's first close look at this enigmatic system on the outskirts of our solar system. In a series of papers, the New Horizons team present their analysis of the encounter data downloaded so far: Moore <jats:italic>et al.</jats:italic> present the complex surface features and geology of Pluto and its large moon Charon, including evidence of tectonics, glacial flow, and possible cryovolcanoes. Grundy <jats:italic>et al.</jats:italic> analyzed the colors and chemical compositions of their surfaces, with ices of H <jats:sub>2</jats:sub> O, CH <jats:sub>4</jats:sub> , CO, N <jats:sub>2</jats:sub> , and NH <jats:sub>3</jats:sub> and a reddish material which may be tholins. Gladstone <jats:italic>et al.</jats:italic> investigated the atmosphere of Pluto, which is colder and more compact than expected and hosts numerous extensive layers of haze. Weaver <jats:italic>et al.</jats:italic> examined the small moons Styx, Nix, Kerberos, and Hydra, which are irregularly shaped, fast-rotating, and have bright surfaces. Bagenal <jats:italic>et al.</jats:italic> report how Pluto modifies its space environment, including interactions with the solar wind and a lack of dust in the system. Together, these findings massively increase our understanding of the bodies in the outer solar system. They will underpin the analysis of New Horizons data, which will continue for years to come. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue pp. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6279" page="1284" related-article-type="in-this-issue" vol="351" xlink:href="10.1126/science.aad7055">1284</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad9189">10.1126/science.aad9189</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad8866">10.1126/science.aad8866</jats:related-article> , <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aae0030">10.1126/science.aae0030</jats:related-article> , & <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aad9045">10.1126/science.aad9045</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. No disponible
Designer protein delivery: From natural to engineered affinity-controlled release systems
Malgosia M. Pakulska; Shane Miersch; Molly S. Shoichet
<jats:title>Temporarily caught in a bind</jats:title> <jats:p> When an atom or molecular fragment is covalently bonded, its release is controlled by the rate of degradation of the bond or by the rate of degradation of the matrix or shell material that keeps it trapped. When molecules are held by noncovalent interactions, the affinity of the molecule to its binding site can be tuned by a number of parameters, such as changing pH, temperature, or salt concentration. This makes it possible to finely tune the release profile. Pakulska <jats:italic>et al.</jats:italic> review our increased understanding of these interactions as found in nature, and their increased use for the delivery of molecular agents and therapeutics. </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" related-article-type="in-this-issue" xlink:href="10.1126/science.aac4750">10.1126/science.aac4750</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. No disponible
Durable coatings that repel ice
Z. H. Kafafi
Palabras clave: Multidisciplinary.
Pp. i-1277
Throwing deep
Michael S. Turner
<jats:p>In a galaxy far, far away (a billion light years away, to be more precise), two massive black holes merged. Spacetime twisted, contorted, and rearranged itself in dramatic fashion, and ripples within its very fabric shot out across the cosmos. Occurrences like this happen hourly somewhere in the universe. What is notable is that on Earth, we detected these ripples, an event now known as GW150914. In the fraction of a second that we “heard” black holes shake up spacetime, a new window on the universe was opened where we hope to hear more black holes, cosmic phase transitions, and even the birth of the universe. The last big prediction of general relativity—the existence of gravitational waves—has been directly confirmed, and we now have a new way of advancing our understanding of gravity, the force that shapes our universe.</jats:p>
Palabras clave: Multidisciplinary.
Pp. 1243-1243
News at a glance
<jats:p>A roundup of weekly science policy and related news.</jats:p>
Palabras clave: Multidisciplinary.
Pp. 1244-1246
Giant atom-smasher gears up to chase whiff of new physics
Adrian Cho
<jats:p>Hints of a massive new particle at the Large Hadron Collider have physicists abuzz —and eager to follow up.</jats:p>
Palabras clave: Multidisciplinary.
Pp. 1248-1249