The Outer Shells of Centaurus A
July 3, 2012
What causes the surrounding shells in peculiar galaxy Cen A? In 2002 a fascinating image of peculiar galaxy Centaurus A was released, processed to highlight a faint blue arc indicating an ongoing collision with a smaller galaxy. Another interesting feature of Cen A, however, is the surrounding system of shells, better visible here in this recently released wider pan from the four meter Blanco telescope at Cerro Tololo Inter-American Observatory. Faint shells around galaxies are not unusual and considered by themselves as evidence of a previous galaxy merger, analogous to water ripples on a pond. An unexpected attribute of these shells is the abundance of gas, which should become separated from existing stars during the collision.
Credits: E. Peng and H. Ford (JHU), K. Freeman (ANU), R. White (STScI), CTIO, NOAO, NSF
Credits: E. Peng and H. Ford (JHU), K. Freeman (ANU), R. White (STScI), CTIO, NOAO, NSF
Topics:
Centaurus A/M83 Group, Centaurus A/M83 Group, Extragalactic astronomy, Peculiar galaxies, Peculiar galaxies, Peculiar galaxies, Centaurus constellation, Centaurus constellation, Astronomy, Lenticular galaxies, Lenticular galaxies, Lenticular galaxies, Centaurus A, Centaurus A, Centaurus A, Centaurus A/M83 Group, Centaurus constellation, Galaxy, Galaxy, Galaxy, Cerro Tololo Inter-American Observatory, Cerro Tololo Inter-American Observatory, Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, National Optical Astronomy Observatory, National Optical Astronomy Observatory, Space Telescope Science Institute, Space Telescope Science Institute, Space Telescope Science Institute
