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Merger in M31’s Bulge & 3-D Accretion – A BVRI CCD Study at Kiso –
Published online by Cambridge University Press: 12 April 2016
Abstract
By contrast-enhancing and colour-excess analyses of BV RI CCD images of the central 12’.5 × 12’.5 region of M31 taken with the Kiso 105 cm Schmidt telescope, we found a “face-on” spiral feature of dark clouds, which are associated with Hα spirals. The feature can be understood as being due to accretion of gas clouds from companion galaxies and/or from a merger galaxy in the past 108–9 years.
- Type
- XI. Galaxies
- Information
- International Astronomical Union Colloquium , Volume 148: The Future Utilisation of Schmidt Telescopes , 1995 , pp. 409 - 414
- Copyright
- Copyright © Astronomical Society of the Pacific 1995