Artigo Produção Nacional Revisado por pares

Upper limits on TeV gamma-ray emission from Centaurus A, Vela X-1, Centaurus X-3, and Circinus X-1

1993; IOP Publishing; Volume: 405; Linguagem: Inglês

10.1086/172386

ISSN

1538-4357

Autores

William H. Allen, I. A. Bond, E. Budding, M. J. Conway, A. Daniel, K. B. Fenton, H. Fujii, Z. Fujii, N. Hayashida, K. Hibino, Mitsuhiko Honda, J. E. Humble, S. Kabe, K. Kasahara, T. Kifune, Grant Lythe, A. Masaike, Y. Matsubara, K. Mitsui, Yoshio Miura, M. Mori, Y. Muraki, M. Nagano, T. Nakamura, M. Nishizawa, P. M. Norris, S. Ogio, To. Saito, M. Sakata, H. Sato, Hideyuki Shimizu, M. Spencer, J. R. Storey, T. Tanimori, M. Teshima, S. Torii, A. Wadsworth, Y. Watase, Michael D. Woodhams, Y. Yamamoto, P. C. M. Yock, T. Yuda, The JANZOS Collaboration,

Tópico(s)

Particle Detector Development and Performance

Resumo

view Abstract Citations (12) References (26) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Upper Limits on TeV Gamma-Ray Emission from Centaurus A, Vela X-1, Centaurus X-3, and Circinus X-1 Allen, W. H. ; Bond, I. A. ; Budding, E. ; Conway, M. J. ; Daniel, A. ; Fenton, K. B. ; Fujii, H. ; Fujii, Z. ; Hayashida, N. ; Hibino, K. ; Honda, M. ; Humble, J. E. ; Kabe, S. ; Kasahara, K. ; Kifune, T. ; Lythe, G. D. ; Masaike, A. ; Matsubara, Y. ; Mitsui, K. ; Miura, Y. ; Mori, M. ; Muraki, Y. ; Nagano, M. ; Nakamura, T. ; Nishizawa, M. ; Norris, P. M. ; Ogio, S. ; Saito, To. ; Sakata, M. ; Sato, H. ; Shimizu, H. M. ; Spencer, M. ; Storey, J. R. ; Tanimori, T. ; Teshima, M. ; Torii, S. ; Wadsworth, A. ; Watase, Y. ; Woodhams, M. D. ; Yamamoto, Y. ; Yock, P. C. M. ; Yuda, T. ; JANZOS Collaboration Abstract The active galaxy Centaurus A and the X-ray binary systems Vela X-1, Centaurus X-3, and Circinus X-1 were monitored for VHE gamma-ray emission above 1 TeV with the JANZOs Cerenkov facility during 1988 and 1989. No evidence was found for persistent or episodic emission from any of these objects. Subseqeunt upper limits on the integral fluxes of 2.2 x 10^-11^, 2.8 x 10^-11^, 4.0 x 10^-11^, and 4.2 x 10^-11^ cm^-2^ s^-1^, respectively, were obtained for these objects. These limits are consistent with results of observations made by other groups. Publication: The Astrophysical Journal Pub Date: March 1993 DOI: 10.1086/172386 Bibcode: 1993ApJ...405..554A Keywords: Active Galaxies; Gamma Ray Astronomy; Radiant Flux Density; X Ray Binaries; Luminosity; X Ray Sources; Astrophysics; GALAXIES: INDIVIDUAL NAME: CENTAURUS A; GAMMA RAYS: OBSERVATIONS; STARS: INDIVIDUAL CONSTELLATION NAME: VELA X-1; STARS: INDIVIDUAL CONSTELLATION NAME: CENTAURUS X-3; STARS: INDIVIDUAL CONSTELLATION NAME: CIRCINUS X-1; X-RAYS: GALAXIES; X-RAYS: STARS full text sources ADS | data products SIMBAD (4) NED (1)

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