- importsource = "00280836-2010-07-08.txt"
- Artículo:
Neuroscience: MicroRNA knocks down cocaine
- Autor:
Marina R. Picciotto
- Resumen:
Cocaine abuse results in increased craving for the drug. But in the long run, cocaine intake induces the expression of a microRNA in the brain, and this seems to limit further drug intake.
- Página:
194
- Publicación:
Nature
- Volúmen:
466
- Número:
7303
- Periodo:
8 Julio 2010
- ISSN:
00280836
- SrcID:
00280836-2010-07-08.txt
- Documento número 1206851
- Actualizado el martes, 10 de julio de 2018 11:34:00 a. m.
- Creado el martes, 10 de julio de 2018 11:34:00 a. m.
- Enlace directo
- Artículo:
Quantum electrodynamics: A chink in the armour?
- Autor:
Jeff Flowers
- Resumen:
A measurement of the size of the proton, obtained using spectroscopy of an exotic atomic system, yields a result of unprecedented accuracy — but in disagreement with values obtained by previous methods.
- Página:
195
- Publicación:
Nature
- Volúmen:
466
- Número:
7303
- Periodo:
8 Julio 2010
- ISSN:
00280836
- SrcID:
00280836-2010-07-08.txt
- Documento número 1206852
- Actualizado el martes, 10 de julio de 2018 11:34:00 a. m.
- Creado el martes, 10 de julio de 2018 11:34:00 a. m.
- Enlace directo
- Artículo:
Striatal microRNA controls cocaine intake through CREB signalling
- Autor:
Jonathan A. Hollander
Heh-In Im
Antonio L. Amelio
Jannet Kocerha
Purva Bali
Qun Lu
David Willoughby
Claes Wahlestedt
Michael D. Conkright
Paul J. Kenny
- Resumen:
Extended cocaine taking triggers several structural and functional changes in the brain that may lead to compulsive drug seeking, but the mechanisms that regulate the process are unclear. Here, a microRNA — miR-212 — is identified that is upregulated in the striatum of rats with a history of extended access to cocaine. The authors suggest that miR-212 protects against the development of compulsive drug taking, and that it may act through the CREB protein, a known regulator of the rewarding effects of cocaine.
- Página:
197
- Publicación:
Nature
- Volúmen:
466
- Número:
7303
- Periodo:
8 Julio 2010
- ISSN:
00280836
- SrcID:
00280836-2010-07-08.txt
- Documento número 1206853
- Actualizado el martes, 10 de julio de 2018 11:34:00 a. m.
- Creado el martes, 10 de julio de 2018 11:34:00 a. m.
- Enlace directo
- Artículo:
Structural mechanism of C-type inactivation in K+ channels
- Autor:
Luis G. Cuello
Vishwanath Jogini
D. Marien Cortes
Eduardo Perozo
- Resumen:
K+ channels can convert between conductive and non-conductive forms through mechanisms that range from flicker transitions (which occur in microseconds) to C-type inactivation (which occurs on millisecond to second timescales). Here, the crystal structures are presented of the potassium channel KcsA in an open-inactivated conformation and 'trapped' in several partially open conformations. The structures indicate a molecular basis for C-type inactivation in K+ channels.
- Página:
203
- Publicación:
Nature
- Volúmen:
466
- Número:
7303
- Periodo:
8 Julio 2010
- ISSN:
00280836
- SrcID:
00280836-2010-07-08.txt
- Documento número 1206854
- Actualizado el martes, 10 de julio de 2018 11:34:00 a. m.
- Creado el martes, 10 de julio de 2018 11:34:00 a. m.
- Enlace directo
- Artículo:
A 300-parsec-long jet-inflated bubble around a powerful microquasar in the galaxy NGC 7793
- Autor:
Manfred W. Pakull
Roberto Soria
Christian Motch
- Resumen:
Ultraluminous X-ray sources are the most luminous class of black hole located outside the nuclei of active galaxies. They are often associated with shock-ionized nebulae, though with no evidence of collimated jets. Now, however, it is reported that the large nebula S26 in the nearby galaxy NGC 7793 is powered by a black hole with a pair of collimated jets. The jets seem to be 104 times more energetic than the X-ray emission from the core.
- Página:
209
- Publicación:
Nature
- Volúmen:
466
- Número:
7303
- Periodo:
8 Julio 2010
- ISSN:
00280836
- SrcID:
00280836-2010-07-08.txt
- Documento número 1206855
- Actualizado el martes, 10 de julio de 2018 11:34:00 a. m.
- Creado el martes, 10 de julio de 2018 11:34:00 a. m.
- Enlace directo