NGC5398 - HST - Potw1737a

(c) ESA/Hubble, CC BY 4.0

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Credit: ESA/Hubble & NASA
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4054 x 2024 Pixel (20165938 Bytes)
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Starbursts in NGC 5398

This NASA/ESA Hubble Space Telescope picture shows NGC 5398, a barred spiral galaxy located about 55 million light-years away.

The galaxy is famous for containing an especially extensive HII region, a large cloud composed of ionised hydrogen (or HII, pronounced “H-two”, with H being the chemical symbol for hydrogen and the “II” indicating that the atoms have lost an electron to become ionised). NGC 5398’s cloud is named Tol 89 and sits at the lower left end of the galaxy’s central “bar” of stars, a structure that cuts through the galactic core and funnels material inwards to maintain the star formation occurring there. Tol 86 is conspicuous in being the only large massive star forming complex in the entire galaxy, with an extension of roughly 5000 times 4000 light-years; it contains at least seven young and massive star clusters. The two brightest clumps within Tol 89, which astronomers have named simply “A” and “B”, appear to have undergone two bursts of star-forming activity — “starbursts” — roughly 4 million and less than 3 million years ago respectively. Tol 89-A is thought to contain a number of particularly bright and massive stars known as Wolf-Rayet stars, which are known for their high temperatures and extreme stellar winds.

Credit:

ESA/Hubble & NASA

Coordinates
Position (RA):	14 1 22.06
Position (Dec):	-33° 3' 49.35"
Field of view:	3.38 x 1.69 arcminutes
Orientation:	North is 99.1° right of vertical

Colours & filters Band	Wavelength	Telescope
Optical V	606 nm	Hubble Space Telescope ACS
Optical V	606 nm	Hubble Space Telescope ACS
Optical I	814 nm	Hubble Space Telescope ACS
Optical V	606 nm	Hubble Space Telescope ACS
Optical I	814 nm	Hubble Space Telescope ACS
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Weitere Informationen zur Lizenz des Bildes finden Sie hier. Letzte Aktualisierung: Fri, 26 Jan 2024 11:12:31 GMT


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NGC 5398

NGC 5398 ist eine Balkenspiralgalaxie vom Hubble-Typ SB(rs)dm im Sternbild Zentaur am Südsternhimmel. Sie schätzungsweise 49 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 55.000 Lj. In NGC 5398 befindet sich das riesige Sternentstehungsgebiet Tol 89, welches Gegenstand gegenwärtiger Untersuchungen ist. Dieses Gebiet hat eine Ausdehnung von 5000 mal 4000 Lichtjahren. .. weiterlesen