Multiwavelength Investigation of γ-Ray Source MGRO J1908+06 Emission Using Fermi-LAT, VERITAS and HAWC

The VERITAS Collaboration; The HAWC Collaboration; The Fermi-LAT Collaboration

doi:10.3847/1538-4357/ad698d

Multiwavelength Investigation of γ-Ray Source MGRO J1908+06 Emission Using Fermi-LAT, VERITAS and HAWC

The VERITAS Collaboration, The HAWC Collaboration, The Fermi-LAT Collaboration

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

This paper investigates the origin of the γ-ray emission from MGRO J1908+06 in the GeV-TeV energy band. By analyzing the data collected by the Fermi Large Area Telescope, the Very Energetic Radiation Imaging Telescope Array System, and High Altitude Water Cherenkov, with the addition of spectral data previously reported by LHAASO, a multiwavelength study of the morphological and spectral features of MGRO J1908+06 provides insight into the origin of the γ-ray emission. The mechanism behind the bright TeV emission is studied by constraining the magnetic field strength, the source age, and the distance through detailed broadband modeling. Both spectral shape and energy-dependent morphology support the scenario that inverse Compton emission of an evolved pulsar wind nebula associated with PSR J1907+0602 is responsible for the MGRO J1908+06 γ-ray emission with a best-fit true age of T = 22 ± 9 kyr and a magnetic field of B = 5.4 ± 0.8 μG, assuming the distance to the pulsar dPSR = 3.2 kpc.

Original language	English (US)
Article number	61
Journal	Astrophysical Journal
Volume	974
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/ad698d
State	Published - Oct 1 2024

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.3847/1538-4357/ad698d

Cite this

@article{083b9fac6f27408da898c5d38587cc2c,

title = "Multiwavelength Investigation of γ-Ray Source MGRO J1908+06 Emission Using Fermi-LAT, VERITAS and HAWC",

abstract = "This paper investigates the origin of the γ-ray emission from MGRO J1908+06 in the GeV-TeV energy band. By analyzing the data collected by the Fermi Large Area Telescope, the Very Energetic Radiation Imaging Telescope Array System, and High Altitude Water Cherenkov, with the addition of spectral data previously reported by LHAASO, a multiwavelength study of the morphological and spectral features of MGRO J1908+06 provides insight into the origin of the γ-ray emission. The mechanism behind the bright TeV emission is studied by constraining the magnetic field strength, the source age, and the distance through detailed broadband modeling. Both spectral shape and energy-dependent morphology support the scenario that inverse Compton emission of an evolved pulsar wind nebula associated with PSR J1907+0602 is responsible for the MGRO J1908+06 γ-ray emission with a best-fit true age of T = 22 ± 9 kyr and a magnetic field of B = 5.4 ± 0.8 μG, assuming the distance to the pulsar dPSR = 3.2 kpc.",

author = "{The VERITAS Collaboration} and {The HAWC Collaboration} and {The Fermi-LAT Collaboration} and A. Acharyya and Adams, {C. B.} and P. Bangale and Bartkoske, {J. T.} and W. Benbow and Buckley, {J. H.} and Christiansen, {J. L.} and Chromey, {A. J.} and A. Duerr and M. Errando and A. Falcone and Q. Feng and Foote, {G. M.} and L. Fortson and A. Furniss and W. Hanlon and D. Hanna and O. Hervet and Hinrichs, {C. E.} and J. Holder and Humensky, {T. B.} and W. Jin and P. Kaaret and M. Kertzman and D. Kieda and Kleiner, {T. K.} and N. Korzoun and S. Kumar and Lang, {M. J.} and M. Lundy and G. Maier and McGrath, {C. E.} and Millard, {M. J.} and J. Millis and Mooney, {C. L.} and P. Moriarty and R. Mukherjee and W. Ning and Ong, {R. A.} and N. Park and M. Pohl and E. Pueschel and J. Quinn and Rabinowitz, {P. L.} and K. Ragan and D. Ribeiro and E. Roache and Ryan, {J. L.} and I. Sadeh and M. Mostaf{\'a}",

note = "Publisher Copyright: {\textcopyright} 2024. The Author(s).",

year = "2024",

month = oct,

day = "1",

doi = "10.3847/1538-4357/ad698d",

language = "English (US)",

volume = "974",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1",

}

TY - JOUR

T1 - Multiwavelength Investigation of γ-Ray Source MGRO J1908+06 Emission Using Fermi-LAT, VERITAS and HAWC

AU - The VERITAS Collaboration

AU - The HAWC Collaboration

AU - The Fermi-LAT Collaboration

AU - Acharyya, A.

AU - Adams, C. B.

AU - Bangale, P.

AU - Bartkoske, J. T.

AU - Benbow, W.

AU - Buckley, J. H.

AU - Christiansen, J. L.

AU - Chromey, A. J.

AU - Duerr, A.

AU - Errando, M.

AU - Falcone, A.

AU - Feng, Q.

AU - Foote, G. M.

AU - Fortson, L.

AU - Furniss, A.

AU - Hanlon, W.

AU - Hanna, D.

AU - Hervet, O.

AU - Hinrichs, C. E.

AU - Holder, J.

AU - Humensky, T. B.

AU - Jin, W.

AU - Kaaret, P.

AU - Kertzman, M.

AU - Kieda, D.

AU - Kleiner, T. K.

AU - Korzoun, N.

AU - Kumar, S.

AU - Lang, M. J.

AU - Lundy, M.

AU - Maier, G.

AU - McGrath, C. E.

AU - Millard, M. J.

AU - Millis, J.

AU - Mooney, C. L.

AU - Moriarty, P.

AU - Mukherjee, R.

AU - Ning, W.

AU - Ong, R. A.

AU - Park, N.

AU - Pohl, M.

AU - Pueschel, E.

AU - Quinn, J.

AU - Rabinowitz, P. L.

AU - Ragan, K.

AU - Ribeiro, D.

AU - Roache, E.

AU - Ryan, J. L.

AU - Sadeh, I.

AU - Mostafá, M.

PY - 2024/10/1

Y1 - 2024/10/1

N2 - This paper investigates the origin of the γ-ray emission from MGRO J1908+06 in the GeV-TeV energy band. By analyzing the data collected by the Fermi Large Area Telescope, the Very Energetic Radiation Imaging Telescope Array System, and High Altitude Water Cherenkov, with the addition of spectral data previously reported by LHAASO, a multiwavelength study of the morphological and spectral features of MGRO J1908+06 provides insight into the origin of the γ-ray emission. The mechanism behind the bright TeV emission is studied by constraining the magnetic field strength, the source age, and the distance through detailed broadband modeling. Both spectral shape and energy-dependent morphology support the scenario that inverse Compton emission of an evolved pulsar wind nebula associated with PSR J1907+0602 is responsible for the MGRO J1908+06 γ-ray emission with a best-fit true age of T = 22 ± 9 kyr and a magnetic field of B = 5.4 ± 0.8 μG, assuming the distance to the pulsar dPSR = 3.2 kpc.

AB - This paper investigates the origin of the γ-ray emission from MGRO J1908+06 in the GeV-TeV energy band. By analyzing the data collected by the Fermi Large Area Telescope, the Very Energetic Radiation Imaging Telescope Array System, and High Altitude Water Cherenkov, with the addition of spectral data previously reported by LHAASO, a multiwavelength study of the morphological and spectral features of MGRO J1908+06 provides insight into the origin of the γ-ray emission. The mechanism behind the bright TeV emission is studied by constraining the magnetic field strength, the source age, and the distance through detailed broadband modeling. Both spectral shape and energy-dependent morphology support the scenario that inverse Compton emission of an evolved pulsar wind nebula associated with PSR J1907+0602 is responsible for the MGRO J1908+06 γ-ray emission with a best-fit true age of T = 22 ± 9 kyr and a magnetic field of B = 5.4 ± 0.8 μG, assuming the distance to the pulsar dPSR = 3.2 kpc.

UR - http://www.scopus.com/inward/record.url?scp=85206322692&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85206322692&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/ad698d

DO - 10.3847/1538-4357/ad698d

M3 - Article

AN - SCOPUS:85206322692

SN - 0004-637X

VL - 974

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 61

ER -

Multiwavelength Investigation of γ-Ray Source MGRO J1908+06 Emission Using Fermi-LAT, VERITAS and HAWC

Abstract

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this