Skip to main content

and
  1. No Access

    Book

  2. No Access

    Article

    Detection of the new rotating radio transient pulsar PSR J2225+35

    We have detected the new pulsar PSR J2225+35, which displays the properties of the new class of radio sources “Rotating Radio Transients” (RRATs). RRATs are distinguished by isolated bursts of radio emission a...

    Yu. P. Shitov, A. D. Kuzmin, D. V. Dumskii, B. Ya. Losovsky in Astronomy Reports (2009)

  3. No Access

    Article

    Giant pulses of pulsar radio emission

    We present a brief review of observational manifestations of pulsars with giant pulses radio emission, based on the survey of the main properties of known pulsars with giant pulses, including our detection of...

    A. D. Kuzmin in Astrophysics and Space Science (2007)

  4. No Access

    Chapter and Conference Paper

    Giant pulses of pulsar radio emission

    We present a brief review of observational manifestations of pulsars with giant pulses radio emission, based on the survey of the main properties of known pulsars with giant pulses, including our detection of ...

    A. D. Kuzmin in Isolated Neutron Stars: From the Surface to the Interior (2007)

  5. No Access

    Article

    Detection of giant radio pulses from the pulsar PSR B0656+14

    Giant pulses (GPs) have been detected from the pulsar PSR B0656 + 14. A pulse that is more intense than the average pulse by a factor of 120 is encountered approximately once in 3000 observed periods of the pu...

    A. D. Kuzmin, A. A. Ershov in Astronomy Letters (2006)

  6. No Access

    Article

    Detection of giant pulses from the pulsar PSR B0031-07

    Giant pulses have been detected from the pulsar PSR B0031-07. A pulse with an intensity higher than that of the average pulse by a factor of 50 or more is encountered approximately once per 300 observed period...

    A. D. Kuzmin, A. A. Ershov, B. Ya. Losovsky in Astronomy Letters (2004)

  7. No Access

    Article

    Peculiarities of giant pulses from the crab pulsar at frequencies of 594 and 2228 MHz

    We present the results of our simultaneous observations of giant pulses from the Crab pulsar B0531+21 at frequencies of 594 and 2228 MHz with a high (62.5 ns) time resolution. The pulse broadening by scatterin...

    S. V. Kostyuk, V. I. Kondratiev, A. D. Kuzmin, M. V. Popov in Astronomy Letters (2003)

  8. No Access

    Article

    Detection of giant pulses from the pulsar PSR B1112+50

    We detected giant pulses from the pulsar PSR B1112+50. A pulse with an intensity that is a factor of 30 or more higher than the intensity of the average pulse is encountered approximately once in 150 observed ...

    A. A. Ershov, A. D. Kuzmin in Astronomy Letters (2003)

  9. No Access

    Article

    Frequency dependence of the scattering pulse broadening for the Crab pulsar

    We measured the frequency dependence of the pulsar pulse broadening by scattering over a wide frequency range, from 40 to 2228 MHz, based on direct measurements of this parameter using giant pulses from the pu...

    A. D. Kuzmin, V. I. Kondrat’ev, S. V. Kostyuk, B. Ya. Losovsky in Astronomy Letters (2002)

  10. No Access

    Article

    Giant pulses from the millisecond pulsar PSR B1937+214

    We have detected giant pulses from the millisecond pulsar PSR B1937+214 at the lowest frequency of 112 MHz. The observed flux density at the pulse peak is ∼40 000 Jy, which exceeds the average level by a facto...

    A. D. Kuzmin, B. Ya. Losovsky in Astronomy Letters (2002)

  11. No Access

    Article

    Low-frequency flux-density measurements and spectral features of millisecond pulsars

    Radio flux-density measurements for a large sample of millisecond pulsars at a low frequency of 102 MHz are presented. Using higher frequency measurements, we construct their spectra in the frequency range fro...

    A. D. Kuzmin, B. Ya. Losovsky in Astronomy Letters (2000)

  12. No Access

    Article

    Secular evolution of the period and inclination of the magnetic to rotation axis and recycled pulsars

    Statistical analysis has been carried out of the relations between period and the ageP−t c, and the inclination of magnetic to rotation axis to the age α−t cof pulsars have been done.

    A. D. Kuzmin, **nji Wu in Astrophysics and Space Science (1992)

  13. No Access

    Article

    Radio spectra of pulsars

    The results of flux pulsar radioemission measurements at meter wavelengths, made at Pushchino Radio Astronomical Observatory of the Lebedev Physical Institute, are presented. Flux densities at 102, 85, 61 and ...

    V. A. Izvekova, A. D. Kuzmin, V. M. Malofeev in Astrophysics and Space Science (1981)