Credit & Copyright: David Martínez-Delgado (University of Heidelberg),
et al.
Explanation:
NGC
4631 is a spiral galaxy found only 25 million light-years away,
toward the well-trained northern constellation
Canes
Venatici.
Seen ege-on, the galaxy is similar in size to
the Milky Way.
Its distorted wedge shape suggests to
some a cosmic herring and to others its popular moniker,
The Whale Galaxy.
The large galaxy's small, remarkably bright elliptical
companion NGC 4627 lies just above its dusty yellowish core,
but also identifiable are recently
discovered,
faint dwarf galaxies within the halo of NGC 4631.
In fact, the faint extended features below (and above)
NGC 4631 are now recognized as tidal star streams.
The star streams are remnants of a dwarf satellite galaxy
disrupted by repeated encounters with the Whale that began
about 3.5 billion years ago.
Even in nearby galaxies,
the presence of tidal star streams is
predicted by cosmological models of galaxy formation, including the
formation of our own Milky Way.
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Январь Февраль Март Апрель Май Июнь Июль Август Сентябрь Октябрь Ноябрь Декабрь |
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Публикации с ключевыми словами:
NGC 4631 - spiral galaxy - interacting galaxies - спиральная галактика - взаимодействующие галактики
Публикации со словами: NGC 4631 - spiral galaxy - interacting galaxies - спиральная галактика - взаимодействующие галактики | |
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