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New observations of the Geminga pulsar at low radio frequencies

Published online by Cambridge University Press:  20 March 2013

V. M. Malofeev
Affiliation:
Pushchino Radio Astronomy Observatory, 142290, Pushchino, Moscow reg., RUSSIA email: malofeev@prao.ru
O. I. Malov
Affiliation:
Pushchino Radio Astronomy Observatory, 142290, Pushchino, Moscow reg., RUSSIA email: malofeev@prao.ru
S. V. Logvinenko
Affiliation:
Pushchino Radio Astronomy Observatory, 142290, Pushchino, Moscow reg., RUSSIA email: malofeev@prao.ru
D. A. Teplykh
Affiliation:
Pushchino Radio Astronomy Observatory, 142290, Pushchino, Moscow reg., RUSSIA email: malofeev@prao.ru
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Abstract

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New evidence for the detection of Geminga at three low frequencies is presented. The observations were carried out on two sensitive transit radio telescopes in the range 42-112 MHz. We used three new digital receivers to detect the pulses and to obtain dynamic spectra. The exact value of the dispersion measure has been calculated.

Keywords

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013

References

Kniffen, D. A., et al. 1975, Proc. 14th Int. Cosmik Ray Conf., 1, 100Google Scholar
Halpern, J. P. & Holt, S. S. 2005, Nature, 357, 222Google Scholar
Bertsch, D. L., et al. 1992, Nature, 357, 306Google Scholar
Malofeev, V. M. & Malov, O. I. 1997, Nature, 389, 697CrossRefGoogle Scholar
Kuzmin, A. D. & Losovsky, B. Y. a. 1997, Pis'ma AZh, 23, 323Google Scholar
Shitov, Yu. P. & Pugachev, V. D. 1998, New Astronomy, 3, 101Google Scholar
Vats, H. O., Singal, A. K., Deshpande, M. R., et al. 1999, MNRAS, 302, 65Google Scholar
Pellizzoni, A., et al. 2011, MNRAS, 416, 45Google Scholar
Malofeev, V. M., Teplykh, D. A., & Logvinenko, S. V. 2012, Astronomy Reports, 56, 35Google Scholar