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    1. IAJ: Product Reviews
    ... The HDF may be heralded as a milestone in years to come, and the book amply records the moment, but it is disconcerting that some astronomers, apparently unexpectedly, hit so much trouble with merging galaxies and blended images. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/iaj/reviews/rev26n1.html -- 49.0 Кб -- 06.07.1999
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    2. http://star.arm.ac.uk/preprints/2010/558.pdf
    ... Intro duction Stars do not form individually but in groups, with sizes ranging from small star forming regions (SFRs) to the massive superstar clusters seen in merging galaxies (Lada & Lada 2003). ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2010/558.pdf -- 939.7 Кб -- 16.03.2010
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    3. Armagh Observatory
    ... Following orbital decay by gravitational-wave radiation, such binaries are expected to merge at a rate of two or three per thousand years per galaxy. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2012/618.html -- 5.7 Кб -- 26.09.2012
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    4. Strong Gravity in the Vicinity of Supermassive Black Holes - by Eamon Scullion,
    ... Black holes are found at the centres of galaxies which are similar in size to our own Milky Way Galaxy or larger. ... When black holes collide and merge they form supermassive black holes which are events among the most powerful in the universe. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/scholars/iya/news/strong_gravity_in_the_vicin.html -- 12.2 Кб -- 31.12.2009
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    5. Armagh Observatory
    ... In the Galaxy as a whole, our model predicts the current birth rate of DWDs to be 3.21 †Ч 10тИТ2 yrтИТ1, the local density to ... Assuming SNIa are formed from the merger of two CO white dwarfs, the SNIa rate should be 0.0013 yrтИТ1. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2010/563.html -- 6.6 Кб -- 23.07.2010
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    6. http://star.arm.ac.uk/~csj/papers/conference/2002_WD13_merger.ps
    ... Population synthesis studies indicate a merger frequency 2 for the Galaxy of between 2:3 4:4 10 3 y 1 [22], [11]. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/papers/conference/2002_WD13_merger.ps -- 84.7 Кб -- 06.08.2002
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    7. Observations with the Faulkes Telescopes
    ... This galaxy can be found within the constellation Ursa Major and is commonly known as the Pinwheel Galaxy. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~dja/faulkes/M101Nova.html -- 8.2 Кб -- 04.04.2015
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    8. Armagh Observatory
    ... Ia supernovae from double degenerate mergers channel in different star formation ... DD) population in the thin disc of the Galaxy, which we assume to have formed 10 Gyr ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2011/581.html -- 6.9 Кб -- 17.08.2011
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    9. http://star.arm.ac.uk/~ambn/314csj.ps
    ... The merger frequency of double HeWD systems in the Galaxy is theoretically estimated ... merger frequency, we obtain  4  10 2 10 3 for the number of the low-luminosity ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/314csj.ps -- 566.1 Кб -- 08.12.1999
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    10. http://star.arm.ac.uk/~csj/papers/journal/hewd_merger.ps
    ... merger of two white dwarfs; a process that should become increasingly common as the ... The merger frequency of double HeWD systems in the Galaxy is theoret- ically ... Galaxy, which is surprisingly consistent with the number predicted from the merged ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/papers/journal/hewd_merger.ps -- 447.8 Кб -- 29.08.2000
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