Estudio experimental de un transformador de calor por absorción con intercambiadores helicoidales múltiples anidados

Autor: KARLA VARELA MARTINEZ

Publikováno v: Universidad Autónoma del Estado de Morelos
UAEM
Repositorio Institucional de Acceso Abierto de la Universidad Autónoma del Estado de Morelos

El presente documento no cuenta con resumen.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______3056::f2670631ab43aabb131e7f436b8eac6b
http://riaa.uaem.mx/handle/20.500.12055/2003

Four GRB supernovae at redshifts between 0.4 and 0.8. The bursts GRB 071112C, 111228A, 120714B, and 130831A

Autor: Adria C. Updike, J. P. U. Fynbo, David Alexander Kann, Arne Rau, Andrea Rossi, Karla Varela, Patricia Schady, Steve Schulze, K. Takats, A. Nicuesa Guelbenzu, R. Filgas, Thomas Krühler, Jochen Greiner, P. M. J. Afonso, S. Schmidl, S. Klose, M. Tanga

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
instname

Twenty years ago, GRB 980425/SN 1998bw revealed that long gamma-ray bursts (GRBs) are physically associated with broad-lined type-Ic supernovae (SNe). Since then more than 1000 long GRBs have been localized to high angular precision, but only in ~50

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88b5c81a384b780e9619039adb55cafd
http://hdl.handle.net/10261/189618

Circular polarization in the optical afterglow of GRB 121024A

Autor: Fabian Knust, A. J. van der Horst, Gianpiero Tagliaferri, Andreja Gomboc, Richard Willingale, Nial R. Tanvir, S. D. Vergani, V. Sudilovsky, R. Karjalainen, David M. Russell, C. Farina, Stefano Covino, Antonia Rowlinson, Zhi-Ping Jin, Karla Varela, Ralph A. M. J. Wijers, R. L. C. Starling, Ruben Salvaterra, Johan P. U. Fynbo, Jochen Greiner, O. E. Hartoog, Yi-Zhong Fan, J. Elliott, P. T. O'Brien, S. di Serego Alighieri, Michiel Min, Jens Hjorth, S. Klose, Carole Mundell, Kenji Toma, D. Gotz, Elena Pian, J. Gorosabel, Shiho Kobayashi, Patricia Schady, Chryssa Kouveliotou, Andrew J. Levan, K. Wiersema, Sergio Campana, P. A. Curran

Publikováno v: Nature
NASA Astrophysics Data System
Wiersema, K, Covino, S, Toma, K, Van Der Horst, A J, Varela, K, Min, M, Greiner, J, Starling, R L C, Tanvir, N R, Wijers, R A M J, Campana, S, Curran, P A, Fan, Y, Fynbo, J P U, Gorosabel, J, Gomboc, A, Götz, D, Hjorth, J, Jin, Z P, Kobayashi, S, Kouveliotou, C, Mundell, C, O’Brien, P T, Pian, E, Rowlinson, A, Russell, D M, Salvaterra, R, Di Serego Alighieri, S, Tagliaferri, G, Vergani, S D, Elliott, J, Fariña, C, Hartoog, O E, Karjalainen, R, Klose, S, Knust, F, Levan, A J, Schady, P, Sudilovsky, V & Willingale, R 2014, ' Circular polarization in the optical afterglow of GRB 121024A ', Nature, vol. 509, no. 7499, pp. 201-204 . https://doi.org/10.1038/nature13237
Nature, 509(7499), 201-204. Nature Publishing Group

Gamma-ray bursts (GRBs) are most probably powered by collimated relativistic outflows (jets) from accreting black holes at cosmological distances. Bright afterglows are produced when the outflow collides with the ambient medium. Afterglow polarizatio

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c875aedc58e9901646a21cad078fa6e
https://dare.uva.nl/personal/pure/en/publications/circular-polarization-in-the-optical-afterglow-of-grb-121024a(8a62e819-003c-46f8-821e-83b8296081ca).html

Microphysics and dynamics of the gamma-ray burst 121024A

Autor: Axel Weiss, Patricia Schady, Andrea Rossi, H. van Eerten, J. Elliott, J. Bolmer, C. De Breuck, V. Sudilovsky, Arne Rau, C. Delvaux, J. F. Graham, D. A. Kann, C. Agurto, Thomas Krühler, A. Nicuesa Guelbenzu, Frank Bertoldi, P. Wiseman, Frederic Schuller, Karla Varela, S. Schmidl, S. Klose, A. J. van der Horst, Jochen Greiner, Fabian Knust, Karl M. Menten, Friedrich Wyrowski, Tassilo Schweyer, R. Filgas, F. Azagra, Arnaud Belloche, M. Tanga

Publikováno v: Varela, K, van Eerten, H, Greiner, J, Schady, P, Elliott, J, Sudilovsky, V, Krühler, T, van der Horst, A J, Bolmer, J, Knust, F, Agurto, C, Azagra, F, Belloche, A, Bertoldi, F, De Breuck, C, Delvaux, C, Filgas, R, Graham, J F, Kann, D A, Klose, S, Menten, K M, Nicuesa Guelbenzu, A, Rau, A, Rossi, A, Schmidl, S, Schuller, F, Schweyer, T, Tanga, M, Weiss, A, Wiseman, P & Wyrowski, F 2016, ' Microphysics and dynamics of the gamma-ray burst 121024A ', Astronomy & Astrophysics, vol. 589, A37, pp. A37 . https://doi.org/10.1051/0004-6361/201526260, https://doi.org/10.1051/0004-6361/201526260
NASA Astrophysics Data System

Aims. The aim of the study is to constrain the physics of gamma-ray bursts (GRBs) by analysing the multi-wavelength afterglow data set of GRB 121024A that covers the full range from radio to X-rays. Methods. Using multi-epoch broad-band observations

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb2968a521373858656fe56806c970b9
https://purehost.bath.ac.uk/ws/files/148876129/1503.07513v3.pdf

A very luminous magnetar-powered supernova associated with an ultra-long gamma-ray burst

Autor: Jochen Greiner, Jonathan Elliott, P. M. J. Afonso, Felipe Olivares E., Roland Diehl, Patricia Schady, Sylvio Klose, D. Alexander Kann, Chris Ashall, Johan P. U. Fynbo, V. Sudilovsky, Shiho Kobayashi, Karla Varela, C. Delvaux, Adria C. Updike, Hendrik van Eerten, Ana Nicuesa Guelbenzu, Giorgos Leloudas, Stefan Taubenberger, Sandra Savaglio, Tassilo Schweyer, J. Bolmer, S. Schmidl, S. J. Prentice, R. Filgas, Thomas Krühler, Paolo A. Mazzali, M. Tanga, Andrea Rossi, J. F. Graham, Fabian Knust, Elena Pian

Publikováno v: Greiner, J, Mazzali, P A, Kann, D A, Krühler, T, Pian, E, Prentice, S, Olivares E., F, Rossi, A, Klose, S, Taubenberger, S, Knust, F, Afonso, P M J, Ashall, C, Bolmer, J, Delvaux, C, Diehl, R, Elliott, J, Filgas, R, Fynbo, J P U, Graham, J F, Guelbenzu, A N, Kobayashi, S, Leloudas, G, Savaglio, S, Schady, P, Schmidl, S, Schweyer, T, Sudilovsky, V, Tanga, M, Updike, A C, van Eerten, H & Varela, K 2015, ' A very luminous magnetar-powered supernova associated with an ultra-long ϒ-ray burst ', Nature, vol. 523, no. 7559, pp. 189-192 . https://doi.org/10.1038/nature14579

A new class of ultra-long duration (>10,000 s) gamma-ray bursts has recently been suggested. They may originate in the explosion of stars with much larger radii than normal long gamma-ray bursts or in the tidal disruptions of a star. No clear superno

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fe9cd7891641f7dbb5af99656faed3bc
http://arxiv.org/abs/1509.03279