ESO 510-G13

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Galaxie
ESO 510-G13
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Warped galaxy.jpg
The spiral galaxy ESO 510-G13, photographed by HST
AladinLite
Constellation Water snake
Position
equinoxJ2000.0 , epoch : J2000.0
Right ascension 13 h 55 m 04.3 s
declination -26 ° 46 ′ 50 ″
Appearance
Morphological type Sa: / pec / sp  
Brightness  (B-band) 13.4 mag
Angular expansion 1.9 ′ × 1.3 ′
Physical data
Redshift 0.011525 ± 0.000030  
Radial velocity 3455 ± 9 km / s  
Stroke distance
v rad  / H 0
(149 ± 10)  x  10 6  ly
(45.8 ± 3.2)  Mpc 
history
Catalog names
PGC  49473 • ESO  510-G13 • MCG  -04-33-013 • IRAS  13522-2632 • AM 1352-263 • PRC D-43

ESO 510-G13 is a 150 million light-years distant spiral galaxy in the constellation Hydra . Its dust disc, which can be seen at the edge , is very noticeably bent, which indicates that it interacted with another galaxy . This structure is particularly emphasized by the dark clouds lying in the disk , which are in front of the stars of the extensive, bright bulges . This conspicuous warp of the disk was first detected by the European Southern Observatory in Chile and is quite unusual, as it normally does not occur in the star-rich inner galactic disk, but in star-poor outer areas consisting of neutral hydrogen . The exact cause of the severely bent glass on the ESO 510-G13 is not known. It could either be the result of a galaxy of the same size or the remnant of the merger with a smaller galaxy.

In the outskirts of the disc are in star-forming regions , many young blue giant stars , which has a high rate of star formation show. This starburst was possibly also stimulated by a galaxy collision, which compressed the interstellar matter .

Web links

Individual evidence

  1. a b c d NASA / IPAC EXTRAGALACTIC DATABASE
  2. a b SEDS : NGC 5000
  3. a b Hubble Photographs Warped Galaxy as Camera Passes Milestone. In: HubbleSite. Space Telescope Science Institute (STScI), August 2, 2001, accessed January 17, 2010 .
  4. Why does ESO 510-G13 have that funny shape? In: Hubble Heritage Project. Space Telescope Science Institute (STScI), accessed January 17, 2010 .