Detalles Bibliográficos
| Autores: |
Albert, Andrea,
Alfaro Molina, José Rubén,
Álvarez Ochoa, César,
Ángeles Camacho, José Roberto,
Araya Arguedas, Miguel,
Arteaga Velázquez, Juan Carlos,
Arun Babu, Kollamparambil Paul,
Ávila Rojas, Daniel Omar,
Ayala Solares, Hugo Alberto,
Baghmanyan, Vardan,
Belmont Moreno, Ernesto,
Brisbois, Chad,
Caballero Mora, Karen Salomé,
Carramiñana, Alberto,
Casanova, Sabrina,
Cotti Gollini, Umberto,
De la Fuente Acosta, Eduardo,
De León Acuña, Cederik León,
Diaz Hernández, Raquel,
Dingus, Brenda L.,
DuVernois, Michael A.,
Durocher, Mora,
Díaz Vélez, Juan Carlos,
Espinoza Hernández, María Catalina,
Fleischhack, Henrike,
Fraija Cabrera, Nissim Illich,
Galván Gámez, Antonio,
García, Distefano,
García González, José Andrés,
Garfias, Fernando,
González, María Magdalena,
Goodman, Jordán Alvin,
Harding, J. Patrick,
Hona, Binita,
Huang, Dezhi,
Hueyotl Zahuantitla, Filiberto,
Hüntemeyer, Petra,
Iriarte, Arturo,
Jardin Blicq, Armelle,
Joshi, Vikas,
León Vargas, Hermes,
Linnemann, James T.,
Longinotti, Anna Lía,
López Coto, Rubén,
Luis Raya, Gilgamesh,
Lundeen, Joseph,
Malone, Kelly,
Martínez Bravo, Oscar Mario,
Martínez Castro, Jesús Alberto,
Matthews, John A.,
Miranda Romagnoli, Pedro,
Moreno Barbosa, Eduardo,
Mostafá, Miguel Alejandro,
Nellen, Lukas,
Nisa, Mehr Un,
Noriega Papaqui, Roberto,
Omodei, Nicola,
Peisker, Alison,
Pérez Pérez, Eucario Gonzalo,
Rho, Chang Dong,
Rosa González, Daniel,
Salesa Greus, Francisco,
Sandoval, Andrés,
Schneider, Michael,
Springer, Robert Wayne,
Tollefson, Kirsten Anne,
Torres Aguilar, Ibrahim Daniel,
Torres Escobedo, Ramiro,
Ureña Mena, Fernando Josué,
Villaseñor Cendejas, Luis Manuel,
Weisgarber, Thomas,
Willox, Elijah Job,
Zepeda, Arnulfo,
Zhou, Hao |
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| Formato: | artículo original
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| Fecha de Publicación: | 2020 |
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| Descripción: | The discovery of the TeV point source 2HWC J2006+341 was reported in the second HAWC gamma-ray catalog. We present a follow-up study of this source here. The TeV emission is best described by an extended source with a soft spectrum. At GeV energies, an extended source is significantly detected in Fermi-LAT data. The matching locations, sizes, and spectra suggest that both gamma-ray detections correspond to the same source. Different scenarios for the origin of the emission are considered and we rule out an association to the pulsar PSR J2004+3429 due to extreme energetics required, if located at a distance of 10.8 kpc. |
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| País: | Kérwá |
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| Institución: | Universidad de Costa Rica |
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| Repositorio: | Kérwá |
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| Lenguaje: | Inglés |
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| OAI Identifier: | oai:kerwa.ucr.ac.cr:10669/90560 |
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| Acceso en línea: | https://iopscience.iop.org/article/10.3847/2041-8213/abbfae
https://hdl.handle.net/10669/90560
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| Palabra clave: | PHYSICS
ULTRAVIOLET RADIATION
GAMMA RAYS
INTERSTELLAR MEDIUM |
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