Paired And Interacting Galaxies : International Astronomical Union Colloquium No. 124
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The luminosity of the ring system given in Table 1 is a lower limit to the total luminosity. However, the absolute magnitude of the rings must be increased by ~1 because of projection effects.
The resulting M(HI)/L Bo ratio is then ~0 . 5 . This value is typical for late type spirals.
Origin of Polar Rings The body of available data, i.e., the size of the rings, their luminosity, mean colors, value of M(HI)/L Bo , and presence of large-scale magntic fields (Hagen-Thorn , Popov, and Yakovleva, 1...979) lead to the conclusion that the system of rings is a spiral 236 galaxy. This conclusion is supported by the fact that luminous rings and dust lines crossing the NE-side of the main body have systematic shifts, which is usual for the arms of spiral galaxies. Therefore the apparent structure of NGC 2685 may be explained as a result of collision of normal SO and Sbc - Sc galaxies.
237 NGC 3808B The Sc galaxy NGC 3808B is a component of an interacting pair with NGC 3808A (W 300, Arp 87). It is located on the end of the spiral arm of NGC 3808A.
What to read after Paired And Interacting Galaxies : International Astronomical Union Colloquium No. 124?
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To quickly assess the difficulty of the text, read a short excerpt:
The luminosity of the ring system given in Table 1 is a lower limit to the total luminosity. However, the absolute magnitude of the rings must be increased by ~1 because of projection effects.
The resulting M(HI)/L Bo ratio is then ~0 . 5 . This value is typical for late type spirals.
Origin of Polar Rings The body of available data, i.e., the size of the rings, their luminosity, mean colors, value of M(HI)/L Bo , and presence of large-scale magntic fields (Hagen-Thorn , Popov, and Yakovleva, 1...979) lead to the conclusion that the system of rings is a spiral 236 galaxy. This conclusion is supported by the fact that luminous rings and dust lines crossing the NE-side of the main body have systematic shifts, which is usual for the arms of spiral galaxies. Therefore the apparent structure of NGC 2685 may be explained as a result of collision of normal SO and Sbc - Sc galaxies.
237 NGC 3808B The Sc galaxy NGC 3808B is a component of an interacting pair with NGC 3808A (W 300, Arp 87). It is located on the end of the spiral arm of NGC 3808A.
What to read after Paired And Interacting Galaxies : International Astronomical Union Colloquium No. 124?
You can find similar books in the "Read Also" column, or choose other free books by University of Alabama to read onlineMoreLess
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