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- W1623897130 abstract "A halo surrounding the edge-on Sb giant spiral galaxy NGC 4565 has been detected in the spectral band 3800–8600 A using a new photometric instrument, an annular scanning photometer. the halo is brightest close to the galactic nucleus and decreases in brightness until it reaches a level of 1 part in 1000 of the sky at a galactic radius of 6.1 arc minutes or 43 kpc from the galactic center. Because the scan path of the ASP is circular, this point corresponds to a distance of 34 kpc from the galactic plane. For comparison, the Holmberg radius of NGC 4565 is equal to 7 arc minutes or 50 kpc. Preliminary V-I photometric data indicate that the halo becomes redder with increasing galactic radius, exceeding V-I = 1.9. Based on a variety of possible origins for the light, it is concluded that the light is due to stars." @default.
- W1623897130 created "2016-06-24" @default.
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- W1623897130 date "1978-01-01" @default.
- W1623897130 modified "2023-10-17" @default.
- W1623897130 title "Detection of an optical halo surrounding the spiral galaxy NGC 4565" @default.
- W1623897130 cites W2017471650 @default.
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- W1623897130 doi "https://doi.org/10.1017/s0074180900144286" @default.
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