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NGC 2550A
NGC 2550A is a spiral galaxy in the constellation of Camelopardalis. Its velocity with respect to the cosmic microwave background is 3670 ± 10 km/s, which corresponds to a Hubble distance of 176.5 ± 12.4 Mly (54.12 ± 3.79 Mpc). The discovery of this galaxy is credited to Philip C. Keenan, in his paper Studies of Extra-Galactic Nebulae. Part I: Determination of Magnitudes, published in The Astrophysical Journal in 1935.
According to A.M. Garcia, NGC 2550A is a member of the NGC 2523 galaxy group (also known as LGG 154). This group contains five galaxies, including NGC 2441, NGC 2523, UGC 4041, and UGC 4199.
Two supernovae have been observed in NGC 2550A:
NGC 2550A
NGC 2550A is a spiral galaxy in the constellation of Camelopardalis. Its velocity with respect to the cosmic microwave background is 3670 ± 10 km/s, which corresponds to a Hubble distance of 176.5 ± 12.4 Mly (54.12 ± 3.79 Mpc). The discovery of this galaxy is credited to Philip C. Keenan, in his paper Studies of Extra-Galactic Nebulae. Part I: Determination of Magnitudes, published in The Astrophysical Journal in 1935.
According to A.M. Garcia, NGC 2550A is a member of the NGC 2523 galaxy group (also known as LGG 154). This group contains five galaxies, including NGC 2441, NGC 2523, UGC 4041, and UGC 4199.
Two supernovae have been observed in NGC 2550A:
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