Spectral Study of Very-high-energy Gamma Rays from SS 433 with HAWC

Authors

R. Alfaro, Universidad Nacional Autónoma de México
C. Alvarez, Universidad Autónoma de Chiapas
J. C. Arteaga-Velázquez, Universidad Michoacana de San Nicolás de Hidalgo
D. Avila Rojas, Universidad Nacional Autónoma de México
H. A. Ayala Solares, Eberly College of Science
R. Babu, Michigan State University
E. Belmont-Moreno, Universidad Nacional Autónoma de México
A. Bernal, Universidad Nacional Autónoma de México
K. S. Caballero-Mora, Universidad Autónoma de Chiapas
T. Capistrán, Universidad Nacional Autónoma de México
A. Carramiñana, Instituto Nacional de Astrofisica Optica y Electronica
S. Casanova, Henryk Niewodniczanski Institute of Nuclear Physics of the Polish Academy of Sciences
J. Cotzomi, Benemérita Universidad Autónoma de Puebla
E. De la Fuente, Universidad de Guadalajara
D. Depaoli, Max-Planck-Institut für Kernphysik
N. Di Lalla, Stanford University
R. Diaz Hernandez, Instituto Nacional de Astrofisica Optica y Electronica
B. L. Dingus, Los Alamos National Laboratory
M. A. DuVernois, UW-Madison College of Engineering
K. Engel, College of Computer, Mathematical, & Natural Sciences
T. Ergin, Michigan State University
C. Espinoza, Universidad Nacional Autónoma de México
K. L. Fan, College of Computer, Mathematical, & Natural Sciences
K. Fang, UW-Madison College of Engineering
N. Fraija, Universidad Nacional Autónoma de México
S. Fraija, Universidad Nacional Autónoma de México
J. A. Garcia-González, Tecnológico de Monterrey
A. Gonzalez Muñoz, Universidad Nacional Autónoma de México
M. M. González, Universidad Nacional Autónoma de México
J. A. Goodman, College of Computer, Mathematical, & Natural Sciences
S. Groetsch, Michigan Technological University

Document Type

Article

Publication Date

11-1-2024

Abstract

Very-high-energy (0.1-100 TeV) gamma-ray emissions were observed in High-Altitude Water Cherenkov (HAWC) data from the lobes of the microquasar SS 433, making them the first set of astrophysical jets that were resolved at TeV energies. In this work, we update the analysis of SS 433 using 2565 days of data from the HAWC observatory. Our analysis reports the detection of a point-like source in the east lobe at a significance of 6.6σ and in the west lobe at a significance of 8.2σ. For each jet lobe, we localize the gamma-ray emission and identify a best-fit position. The locations are close to the X-ray emission sites “e1” and “w1” for the east and west lobes, respectively. We analyze the spectral energy distributions and find that the energy spectra of the lobes are consistent with a simple power law d N/d E ∝ E α with α = − 2.44 − 0.12 − 0.04 + 0.13 + 0.04 and α = − 2.35 − 0.11 − 0.03 + 0.12 + 0.03 for the east and west lobes, respectively. The maximum energy of photons from the east and west lobes reaches 56 TeV and 123 TeV, respectively. We compare our observations to various models and conclude that the very-high-energy gamma-ray emission can be produced by a population of electrons that were efficiently accelerated.

Publication Title

Astrophysical Journal

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