Noutsos A, Abdo AA, Ackermann M, Ajello M, Ballet J, Barbiellini G, Baring MG, Bastieri D, Bechtol K, Bellazzini R, Berenji B, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Buehler R, Busetto G, Caliandro GA, Cameron RA, Camilo F, Caraveo PA, Casandjian JM, Cecchi C, Celik O, Chaty S, Chekhtman A, Chiang J, Ciprini S, Claus R, Cognard I, Cohen-Tanugi J, Colafrancesco S, Cutini S, Dermer CD, De Palma F, Drell PS, Dumora D, Ea CM, Favuzzi C, Ferrara EC, Focke WB, Frailis M, Freire PCC, Fukazawa Y, Funk S, Fusco P, Gargano F, Germani S, Giglietto N, Giordano F, Giroletti M, Godfrey G, Grandi P, Grenier IA, Grove JE, Guillemot L, Guiriec S, Harding AK, Hughes RE, Jackson MS, Johannesson G, Johnson AS, Johnson TJ, Johnson WN, Johnston S, Kamae T, Katagiri H, Kataoka J, Knoedlseder J, Kramer M, Kuss MW, Lande J, Lee SH, Longo F, Loparco F, Lovellette MN, Lubrano P, Lyne AG, Makeev A, Marelli M, Mazziotta MN, Mcenery JE, Mehault J, Michelson PF, Mizuno T, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Naumann-Godo M, Nolan PL, Nuss E, Ohsugi T, Okumura A, Omodei N, Orlando E, Ormes JF, Panetta JH, Parent D, Pelassa V, Pepe M, Persic M, Pesce-Rollins M, Piron F, Porter TA, Raino S, Ray PS, Razzano M, Reimer A, Reimer O, Reposeur T, Romani RW, Sadrozinski HFW, Sander A, Parkinson PMS, Sgro C, Siskind EJ, Smith DA, Smith PD, Spandre G, Spinelli P, Stappers BW, Strickman MS, Suson DJ, Takahashi HH, Tanaka T, Theureau G, Thompson DJ, Thorsett SE, Tibolla O, Torres DF, Tramacere A, Usher TL, Vandenbroucke J, Vianello G, Vilchez N, Villata M, Vitale V, Von Kienlin A, Waite AP, Wang P, Watters K, Weltevrede P, Winer BL, Wood KS, Ziegler M (2011)
Publication Type: Journal article
Publication year: 2011
Book Volume: 728
Journal Issue: 2
DOI: 10.1088/0004-637X/728/2/77
We report on the first year of Fermi gamma-ray observations of pulsed high-energy emission from the old PSR J2043 + 2740. The study of the gamma-ray efficiency of such old pulsars gives us an insight into the evolution of pulsars' ability to emit in gamma rays as they age. The gamma-ray light curve of this pulsar above 0.1 GeV is clearly defined by two sharp peaks, 0.353 +/- 0.035 periods apart. We have combined the gamma-ray profile characteristics of PSR J2043 + 2740 with the geometrical properties of the pulsar's radio emission, derived from radio-polarization data, and constrained the pulsar-beam geometry in the framework of a two-pole caustic (TPC) and an outer gap (OG) model. The ranges of magnetic inclination and viewing angle were determined to be {alpha, zeta} similar to {52 degrees-57 degrees, 61 degrees-68 degrees} for the TPC model, and {alpha, zeta} similar to {62 degrees-73 degrees, 74 degrees-81 degrees} and {alpha, zeta} similar to {72 degrees-83 degrees, 60 degrees-75 degrees} for the OG model. Based on this geometry, we assess possible birth locations for this pulsar and derive a likely proper motion, sufficiently high to be measurable with VLBI. At a characteristic age of 1.2 Myr, PSR J2043 + 2740 is the third oldest of all discovered, non-recycled, gamma-ray pulsars: it is twice as old as the next oldest, PSR J0357 + 32, and younger only than the recently discovered PSR J1836 + 5925 and PSR J2055 + 25, both of which are at least five and ten times less energetic, respectively.
APA:
Noutsos, A., Abdo, A.A., Ackermann, M., Ajello, M., Ballet, J., Barbiellini, G.,... Ziegler, M. (2011). RADIO AND gamma-RAY CONSTRAINTS ON THE EMISSION GEOMETRY AND BIRTHPLACE OF PSR J2043+2740. Astrophysical Journal, 728(2). https://doi.org/10.1088/0004-637X/728/2/77
MLA:
Noutsos, A., et al. "RADIO AND gamma-RAY CONSTRAINTS ON THE EMISSION GEOMETRY AND BIRTHPLACE OF PSR J2043+2740." Astrophysical Journal 728.2 (2011).
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