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Analysis of the Emission and Morphology of the Pulsar Wind Nebula Candidate HAWC J2031+415

Fuente: arXiv
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Autori principali: Alfaro, R., Alvarez, C., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Babu, R., Belmont-Moreno, E., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Cotti, U., Cotzomi, J., de León, S. Coutiño, De la Fuente, E., de León, C., Depaoli, D., Di Lalla, N., Hernandez, R. Diaz, Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Engel, K., Ergin, T., Espinoza, C., Fan, K. L., Fraija, N., García-González, J. A., González, M. M., Goodman, J. A., Groetsch, S., Harding, J. P., Hernández-Cadena, S., Herzog, I., Huang, D., Hueyotl-Zahuantitla, F., Hüntemeyer, P., Iriarte, A., Kaufmann, S., Lee, J., Vargas, H. León, Longinotti, A. L., Luis-Raya, G., Malone, K., Martínez-Castro, J., Matthews, J. A., Miranda-Romagnoli, P., Montes, . A., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Araujo, Y. Pérez, Pérez-Pérez, E. G., Rho, C. D., Rosa-González, D., Ruiz-Velasco, E., Salazar, H., Salazar-Gallegos, D., Sandoval, A., Schneider, M., Serna-Franco, J., Smith, A. J., Son, Y., Springer, R. W., Tibolla, O., Tollefson, K., Torres, I., Torres-Escobedo, R., Turner, R., Ureña-Mena, F., Varela, E., Villaseñor, L., Wang, X., Wang, Zhen, Watson, I. J., Yu, S., Yun-Cárcamo, S., Zhou, H.
Natura: Preprint
Pubblicazione: 2024
Soggetti:
High Energy Astrophysical Phenomena
High Energy Physics - Experiment
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author Alfaro, R.
Alvarez, C.
Arteaga-Velázquez, J. C.
Rojas, D. Avila
Solares, H. A. Ayala
Babu, R.
Belmont-Moreno, E.
Caballero-Mora, K. S.
Capistrán, T.
Carramiñana, A.
Casanova, S.
Cotti, U.
Cotzomi, J.
de León, S. Coutiño
De la Fuente, E.
de León, C.
Depaoli, D.
Di Lalla, N.
Hernandez, R. Diaz
Dingus, B. L.
DuVernois, M. A.
Díaz-Vélez, J. C.
Engel, K.
Ergin, T.
Espinoza, C.
Fan, K. L.
Fraija, N.
García-González, J. A.
González, M. M.
Goodman, J. A.
Groetsch, S.
Harding, J. P.
Hernández-Cadena, S.
Herzog, I.
Huang, D.
Hueyotl-Zahuantitla, F.
Hüntemeyer, P.
Iriarte, A.
Kaufmann, S.
Lee, J.
Vargas, H. León
Longinotti, A. L.
Luis-Raya, G.
Malone, K.
Martínez-Castro, J.
Matthews, J. A.
Miranda-Romagnoli, P.
Montes, . A.
Moreno, E.
Mostafá, M.
Nellen, L.
Newbold, M.
Nisa, M. U.
Noriega-Papaqui, R.
Araujo, Y. Pérez
Pérez-Pérez, E. G.
Rho, C. D.
Rosa-González, D.
Ruiz-Velasco, E.
Salazar, H.
Salazar-Gallegos, D.
Sandoval, A.
Schneider, M.
Serna-Franco, J.
Smith, A. J.
Son, Y.
Springer, R. W.
Tibolla, O.
Tollefson, K.
Torres, I.
Torres-Escobedo, R.
Turner, R.
Ureña-Mena, F.
Varela, E.
Villaseñor, L.
Wang, X.
Wang, Zhen
Watson, I. J.
Yu, S.
Yun-Cárcamo, S.
Zhou, H.
author_facet Alfaro, R.
Alvarez, C.
Arteaga-Velázquez, J. C.
Rojas, D. Avila
Solares, H. A. Ayala
Babu, R.
Belmont-Moreno, E.
Caballero-Mora, K. S.
Capistrán, T.
Carramiñana, A.
Casanova, S.
Cotti, U.
Cotzomi, J.
de León, S. Coutiño
De la Fuente, E.
de León, C.
Depaoli, D.
Di Lalla, N.
Hernandez, R. Diaz
Dingus, B. L.
DuVernois, M. A.
Díaz-Vélez, J. C.
Engel, K.
Ergin, T.
Espinoza, C.
Fan, K. L.
Fraija, N.
García-González, J. A.
González, M. M.
Goodman, J. A.
Groetsch, S.
Harding, J. P.
Hernández-Cadena, S.
Herzog, I.
Huang, D.
Hueyotl-Zahuantitla, F.
Hüntemeyer, P.
Iriarte, A.
Kaufmann, S.
Lee, J.
Vargas, H. León
Longinotti, A. L.
Luis-Raya, G.
Malone, K.
Martínez-Castro, J.
Matthews, J. A.
Miranda-Romagnoli, P.
Montes, . A.
Moreno, E.
Mostafá, M.
Nellen, L.
Newbold, M.
Nisa, M. U.
Noriega-Papaqui, R.
Araujo, Y. Pérez
Pérez-Pérez, E. G.
Rho, C. D.
Rosa-González, D.
Ruiz-Velasco, E.
Salazar, H.
Salazar-Gallegos, D.
Sandoval, A.
Schneider, M.
Serna-Franco, J.
Smith, A. J.
Son, Y.
Springer, R. W.
Tibolla, O.
Tollefson, K.
Torres, I.
Torres-Escobedo, R.
Turner, R.
Ureña-Mena, F.
Varela, E.
Villaseñor, L.
Wang, X.
Wang, Zhen
Watson, I. J.
Yu, S.
Yun-Cárcamo, S.
Zhou, H.
contents The first TeV gamma-ray source with no lower energy counterparts, TeV J2032+4130, was discovered by HEGRA. It appears in the third HAWC catalog as 3HWC J2031+415 and it is a bright TeV gamma-ray source whose emission has previously been resolved as 2 sources: HAWC J2031+415 and HAWC J2030+409. While HAWC J2030+409 has since been associated with the \emph{Fermi-LAT} Cygnus Cocoon, no such association for HAWC J2031+415 has yet been found. In this work, we investigate the spectrum and energy-dependent morphology of HAWC J2031+415. We associate HAWC J2031+415 with the pulsar PSR J2032+4127 and perform a combined multi-wavelength analysis using radio, X-ray, and $γ$-ray emission. We conclude that HAWC J2031+415 and, by extension, TeV J2032+4130 are most probably a pulsar wind nebula (PWN) powered by PSR J2032+4127.
format Preprint
id arxiv_https___arxiv_org_abs_2407_02879
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Analysis of the Emission and Morphology of the Pulsar Wind Nebula Candidate HAWC J2031+415
Alfaro, R.
Alvarez, C.
Arteaga-Velázquez, J. C.
Rojas, D. Avila
Solares, H. A. Ayala
Babu, R.
Belmont-Moreno, E.
Caballero-Mora, K. S.
Capistrán, T.
Carramiñana, A.
Casanova, S.
Cotti, U.
Cotzomi, J.
de León, S. Coutiño
De la Fuente, E.
de León, C.
Depaoli, D.
Di Lalla, N.
Hernandez, R. Diaz
Dingus, B. L.
DuVernois, M. A.
Díaz-Vélez, J. C.
Engel, K.
Ergin, T.
Espinoza, C.
Fan, K. L.
Fraija, N.
García-González, J. A.
González, M. M.
Goodman, J. A.
Groetsch, S.
Harding, J. P.
Hernández-Cadena, S.
Herzog, I.
Huang, D.
Hueyotl-Zahuantitla, F.
Hüntemeyer, P.
Iriarte, A.
Kaufmann, S.
Lee, J.
Vargas, H. León
Longinotti, A. L.
Luis-Raya, G.
Malone, K.
Martínez-Castro, J.
Matthews, J. A.
Miranda-Romagnoli, P.
Montes, . A.
Moreno, E.
Mostafá, M.
Nellen, L.
Newbold, M.
Nisa, M. U.
Noriega-Papaqui, R.
Araujo, Y. Pérez
Pérez-Pérez, E. G.
Rho, C. D.
Rosa-González, D.
Ruiz-Velasco, E.
Salazar, H.
Salazar-Gallegos, D.
Sandoval, A.
Schneider, M.
Serna-Franco, J.
Smith, A. J.
Son, Y.
Springer, R. W.
Tibolla, O.
Tollefson, K.
Torres, I.
Torres-Escobedo, R.
Turner, R.
Ureña-Mena, F.
Varela, E.
Villaseñor, L.
Wang, X.
Wang, Zhen
Watson, I. J.
Yu, S.
Yun-Cárcamo, S.
Zhou, H.
High Energy Astrophysical Phenomena
High Energy Physics - Experiment
The first TeV gamma-ray source with no lower energy counterparts, TeV J2032+4130, was discovered by HEGRA. It appears in the third HAWC catalog as 3HWC J2031+415 and it is a bright TeV gamma-ray source whose emission has previously been resolved as 2 sources: HAWC J2031+415 and HAWC J2030+409. While HAWC J2030+409 has since been associated with the \emph{Fermi-LAT} Cygnus Cocoon, no such association for HAWC J2031+415 has yet been found. In this work, we investigate the spectrum and energy-dependent morphology of HAWC J2031+415. We associate HAWC J2031+415 with the pulsar PSR J2032+4127 and perform a combined multi-wavelength analysis using radio, X-ray, and $γ$-ray emission. We conclude that HAWC J2031+415 and, by extension, TeV J2032+4130 are most probably a pulsar wind nebula (PWN) powered by PSR J2032+4127.
title Analysis of the Emission and Morphology of the Pulsar Wind Nebula Candidate HAWC J2031+415
topic High Energy Astrophysical Phenomena
High Energy Physics - Experiment
url https://arxiv.org/abs/2407.02879

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