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Multiwavelength observations of markarian 421 during a tev/x-ray flare

  • D. J. Macomb
  • , C. W. Akerlof
  • , H. D. Aller
  • , M. F. Aller
  • , D. L. Bertsch
  • , F. Bruhweiler
  • , J. H. Buckley
  • , D. A. Carter-Lewis
  • , M. F. Cawley
  • , K. P. Cheng
  • , C. Dermer
  • , D. J. Fegan
  • , J. A. Gaidos
  • , W. K. Gear
  • , C. R. Hall
  • , R. C. Hartman
  • , A. M. Hillas
  • , M. Kafatos
  • , A. D. Kerrick
  • , D. A. Kniffen
  • Y. Kondo, H. Kubo, R. C. Lamb, F. Makino, K. Makishima, A. Marscher, J. McEnery, I. M. McHardy, D. I. Meyer, E. M. Moore, E. Ramos, E. I. Robson, H. J. Rose, M. S. Schubnell, G. Sembroski, J. A. Stevens, T. Takahashi, M. Tashiro, T. C. Weekes, C. Wilson, J. Zweerink
  • University of Michigan, Ann Arbor
  • NASA Goddard Space Flight Center
  • Catholic University of America
  • Harvard-Smithsonian CfA
  • Iowa State University
  • St. Patrick's College
  • Naval Research Laboratory
  • University College Dublin
  • Purdue University
  • Royal Observatory
  • University of Leeds
  • George Mason University
  • Hampden-Sydney College
  • The University of Tokyo
  • JAXA Institute of Space and Astronautical Science
  • Boston University
  • University of Southampton
  • University of Hawai'i at Mānoa
  • University of Central Lancashire

Research output: Contribution to journalArticlepeer-review

149 Scopus citations

Abstract

A TeV flare from the BL Lac object Mrk 421 was detected in May of 1994 by the Whipple Observatory air Cherenkov experiment during which the flux above 250 GeV increased by nearly an order of magnitude over a 2-day period. Contemporaneous observations by ASCA showed the X-ray flux to be in a very high state. We present these results, combined with the first ever simultaneous or nearly simultaneous observations at GeV gamma-ray, UV, IR, mm, and radio energies for this nearest BL Lac object. While the GeV gamma-ray flux increased slightly, there is little evidence for variability comparable to that seen at TeV and X-ray energies. other wavelengths show even less variability. This provides important constraints on the emission mechanisms at work. We present the multiwavelength spectrum of this gamma-ray blazar for both quiescent and flaring states and discuss the data in terms of current models of blazar emission.

Original languageEnglish
Pages (from-to)L99-L103
JournalAstrophysical Journal
Volume449
Issue number2
DOIs
StatePublished - 20 Aug 1995

Keywords

  • BL Lacertae objects: General
  • BL Lacertae objects: Individual (Markarian 421)

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