ПЕРВЫЕ РЕЗУЛЬТАТЫ ДЕКАМЕТРОВОГО ОБЗОРА СЕВЕРНОГО НЕБА. РЕДЕТЕКТИРОВАНИЕ ИЗВЕСТНЫХ ПУЛЬСАРОВ

At the UTR-2 radio telescope the survey of northern sky is being conducted with aim to search for pulsars and transients. In the first stage the detection of a complete list of known pulsars with parameters DM -3, period more than 0.1 s and declination above -10° was carried out. For the first time...

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Main Authors: В. В Захаренко, Я. Ю. Васильева, А. А. Коноваленко, Ф. Зарка, В. С. Николаенко
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2011-12-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/85101
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spelling doaj-ca2875109603496d8bb908a96b9046702020-11-25T03:10:34ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152011-12-0124011711910.18524/1810-4215.2011.24.8510185101ПЕРВЫЕ РЕЗУЛЬТАТЫ ДЕКАМЕТРОВОГО ОБЗОРА СЕВЕРНОГО НЕБА. РЕДЕТЕКТИРОВАНИЕ ИЗВЕСТНЫХ ПУЛЬСАРОВВ. В Захаренко0Я. Ю. ВасильеваА. А. КоноваленкоФ. ЗаркаВ. С. НиколаенкоРадиоастрономический институт НАН УкраиныAt the UTR-2 radio telescope the survey of northern sky is being conducted with aim to search for pulsars and transients. In the first stage the detection of a complete list of known pulsars with parameters DM -3, period more than 0.1 s and declination above -10° was carried out. For the first time in the decameter range more than a half of known pulsars with the aforementioned parameters (40 of 74) have been detected, whereas before there were known only about 10 of them. An average exponent value for the frequency dependence of scattering time constant for the detected pulsars was obtained. It is equal 4.18. Also, the value of the radiation cone broadening was estimated. With decreasing of frequency from 100 to 25 MHz for pulsars with period of < 1 s the extension is equal 2.2, and with period of > 1 s – 1.6 times. Obtained results give a hope for finding a significant number of pulsars and transient sources of radiation in the ongoing survey.http://oap.onu.edu.ua/article/view/85101
collection DOAJ
language English
format Article
sources DOAJ
author В. В Захаренко
Я. Ю. Васильева
А. А. Коноваленко
Ф. Зарка
В. С. Николаенко
spellingShingle В. В Захаренко
Я. Ю. Васильева
А. А. Коноваленко
Ф. Зарка
В. С. Николаенко
ПЕРВЫЕ РЕЗУЛЬТАТЫ ДЕКАМЕТРОВОГО ОБЗОРА СЕВЕРНОГО НЕБА. РЕДЕТЕКТИРОВАНИЕ ИЗВЕСТНЫХ ПУЛЬСАРОВ
Odessa Astronomical Publications
author_facet В. В Захаренко
Я. Ю. Васильева
А. А. Коноваленко
Ф. Зарка
В. С. Николаенко
author_sort В. В Захаренко
title ПЕРВЫЕ РЕЗУЛЬТАТЫ ДЕКАМЕТРОВОГО ОБЗОРА СЕВЕРНОГО НЕБА. РЕДЕТЕКТИРОВАНИЕ ИЗВЕСТНЫХ ПУЛЬСАРОВ
title_short ПЕРВЫЕ РЕЗУЛЬТАТЫ ДЕКАМЕТРОВОГО ОБЗОРА СЕВЕРНОГО НЕБА. РЕДЕТЕКТИРОВАНИЕ ИЗВЕСТНЫХ ПУЛЬСАРОВ
title_full ПЕРВЫЕ РЕЗУЛЬТАТЫ ДЕКАМЕТРОВОГО ОБЗОРА СЕВЕРНОГО НЕБА. РЕДЕТЕКТИРОВАНИЕ ИЗВЕСТНЫХ ПУЛЬСАРОВ
title_fullStr ПЕРВЫЕ РЕЗУЛЬТАТЫ ДЕКАМЕТРОВОГО ОБЗОРА СЕВЕРНОГО НЕБА. РЕДЕТЕКТИРОВАНИЕ ИЗВЕСТНЫХ ПУЛЬСАРОВ
title_full_unstemmed ПЕРВЫЕ РЕЗУЛЬТАТЫ ДЕКАМЕТРОВОГО ОБЗОРА СЕВЕРНОГО НЕБА. РЕДЕТЕКТИРОВАНИЕ ИЗВЕСТНЫХ ПУЛЬСАРОВ
title_sort первые результаты декаметрового обзора северного неба. редетектирование известных пульсаров
publisher Odessa I. I. Mechnykov National University
series Odessa Astronomical Publications
issn 1810-4215
publishDate 2011-12-01
description At the UTR-2 radio telescope the survey of northern sky is being conducted with aim to search for pulsars and transients. In the first stage the detection of a complete list of known pulsars with parameters DM -3, period more than 0.1 s and declination above -10° was carried out. For the first time in the decameter range more than a half of known pulsars with the aforementioned parameters (40 of 74) have been detected, whereas before there were known only about 10 of them. An average exponent value for the frequency dependence of scattering time constant for the detected pulsars was obtained. It is equal 4.18. Also, the value of the radiation cone broadening was estimated. With decreasing of frequency from 100 to 25 MHz for pulsars with period of < 1 s the extension is equal 2.2, and with period of > 1 s – 1.6 times. Obtained results give a hope for finding a significant number of pulsars and transient sources of radiation in the ongoing survey.
url http://oap.onu.edu.ua/article/view/85101
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