Ядерные гамма-линии в исследованиях астрофизических объектов Галактики и Метагалактики тема диссертации и автореферата по ВАК РФ 01.03.02, доктор физико-математических наук Июдин, Анатолий Федорович

  • Июдин, Анатолий Федорович
  • доктор физико-математических наукдоктор физико-математических наук
  • 2013, Санкт-Петербург
  • Специальность ВАК РФ01.03.02
  • Количество страниц 255
Июдин, Анатолий Федорович. Ядерные гамма-линии в исследованиях астрофизических объектов Галактики и Метагалактики: дис. доктор физико-математических наук: 01.03.02 - Астрофизика, радиоастрономия. Санкт-Петербург. 2013. 255 с.

Оглавление диссертации доктор физико-математических наук Июдин, Анатолий Федорович

1 Введение.

1.1 Роль ядерных гамма-линий в астрофизических исследованиях.

2 Комптоновская Гамма-Обсерватория.

2.1 Прибор КОМПТЕЛ — комптоновский гамма-телескоп.

2.1.1 Восстановление энергии и направления регистрируемого гамма-кванта в приборе КОМПТЕЛ.

2.1.2 Условия наблюдений и компоненты фона в приборе КОМПТЕЛ.

2.1.3 Основы анализа регистрируемой информации для прибора КОМПТЕЛ.

2.1.3.1. Пространственный анализ.

2.1.3.2. Спектральный анализ.

2.2 Гамма-телескоп ЭГРЕТ.

2.2.1 Принцип регистрации гамма-квантов прибором ЭГРЕТ.

2.2.2 Восстановление энергии и направления регистрируемого гамма-кванта в приборе ЭГРЕТ.

2.2.3 Основы обработки регистрируемой прибором ЭГРЕТ информации для получения координат и спектра источника гамма-излучения

3 Наблюдения гамма-излучения в линии 1.157 МэВ от остатка сверхновой Кассиопея А.

3.1 Первое наблюдение гамма-линии 1.157 МэВ от остатка сверхновой Кассиопея А.

3.2 Проверка полученного результата регистрации прибором КОМПТЕЛ гамма-линии 1.157 МэВ от остатка сверхновой Кассиопея А.

3.3 Анализ возможных имитаций у-линии 1.157 МэВ зарегистрированной от остатка сверхновой Кассиопея А прибором КОМПТЕЛ.

3.4 Независимое подтверждение регистрации гамма-линий от распада 44Ti от остатка сверхновой Кассиопея А.

3.5 Интерпретация результата регистрации гамма-линии 1.157 МэВ от остатка сверхновой Кассиопея А прибором КОМПТЕЛ.

3.6 Вопрос количества 44Ti в остатке сверхновой Кассиопея А.

3.7 Выводы к материалам Главы 3.

4 Поиск источников излучения в гамма-линии 1.157 МэВ в плоскости Галактики.

4.1 Генерация и анализ первой карты излучения галактики в гамма-линии с энергией 1.157 МэВ по данным прибора КОМПТЕЛ.

4.2 Генерация и анализ конечного варианта карты излучения галактики в у-линии с энергией 1.157 МэВ по данным прибора КОМПТЕЛ.

4.3 Ограничения на частоту сверхновых в Галактике по числу источников зарегистрированных в линии 1.157 МэВ.

5 Исследования свойств молодого галактического остатка сверхновой Vela Jr.

5.1 Свойства остатка сверхновой RX J0852.0-4622.

5.2 Морфологические особенности остатка сверхновой RX J0852.0-4622 по измерениям в других длинах волн и энергиях у-излучения.

5.3 К определению возраста остатка сверхновой RX J0852.0-4622.

5.4 Независимое подтверждение регистрации гамма-линии 1.157 МэВ от остатка сверхновой Vela Jr. прибором КОМПТЕЛ.9з

5.5 Молодой остаток сверхновой Gl.9+0.3 содержащий 44Ti?.

5.6 Молодой остаток сверхновой SN1987A содержащий 44Ti.

5.7 Выводы по остатку сверхновой Vela Jr. содержащей 44Ti.

6. Исследования гамма-излучения в линии 1.275 МэВ от галактических классических новых.

6.1 Результаты исследований гамма-излучения в линии 22Na с энергией 1.275 МэВ от ближайших классических новых вспыхнувших в Галактике в период 1991-1999 г.г.

6.2. Наблюдения линии 1.275 МэВ изотопа 22Na прибором COMPTEL.

6.2.1. Поиск локальных избытков излучения в линии 1.275 МэВ.

6.2.2. Спектральный анализ и поиск излучения в линии 1.275 МэВ.

6.3. Выводы из результатов наблюдений 1991-1994 гг.

6.4. Излучение в линии 1.275 МэВ от Новой Кассиопеи 1995.

Выводы к Главе 6.

7. Галактическое излучение в гамма-линии 1.275 МэВ.

7.1 Результаты исследований глобального галактического излучения в линии с энергией 1.275 МэВ.

7.2 Широтный и долготный профили интенсивности галактического излучения в гамма-линии с энергией 1.275 МэВ.

7.3 Оценка частоты новых в балдже.

7.4 Оценка потока в линии 1.275 МэВ от КЛНЭ в балдже.

Выводы к Главе 7.

8. Метод резонансного поглощения гамма-квантов в исследованиях источников с релятивисткими струями.

8.1 Процессы резонансного поглощения гамма-квантов ядрами межзвездного и межгалактического вещества.

8.2. Краткое описание приборов и методики анализа спектров квазаров. 132 8.2.1. Прибор COMPTEL.

8.2.2. Краткое описание прибора EGRET.

8.2.3.Анализ регистрируемых данных прибора COMPTEL.

8.2.4.Особенности анализа спектров квазаров для прибора EGRET.

8.2.4.1. Стандартный анализ спектров прибора EGRET.

8.2.4.2. Специфика нашего анализа спектров прибора EGRET.

8.3. Спектры квазаров измеренные приборами COMPTEL и EGRET.

8.3. 1. Процесс фитирования спектров квазаров.

8.3.2. Анализ СПИ квазара ЗС279.

8.3.3. Анализ СПИ квазара 3C273.

8.3.4. Анализ СПИ квазара PKS 0528+134.

8.3.5. Анализ СПИ квазара BL Lacertae.

8.4. Возможность практического применения метода резонансного поглощения в исследованиях ранней Вселенной.

Рекомендованный список диссертаций по специальности «Астрофизика, радиоастрономия», 01.03.02 шифр ВАК

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