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BG Canis Minoris is a binary star system in the equatorial constellation of Canis Minor, abbreviated BG CMi. With an apparent visual magnitude that fluctuates around 14.5, [ 3 ] it is much too faint to be visible to the naked eye .
YY Canis Minoris, abbreviated YY CMi and otherwise referred to as HD 67110, is an eclipsing contact binary in the constellation of Canis Minor, close to the border with Hydra. Its apparent magnitude ranges between 8.46 and 9.23, making it too faint to be seen by the naked eye but visible using binoculars . [ 7 ]
It also has the strongest and hardest X-ray emission of any β Cephei star. [6] ξ 1 Canis Majoris forms a naked eye pairing with ξ 2 Canis Majoris a little less than a degree away. The Washington Double Star Catalog lists two 14th magnitude companions about 27″ away. [10]
X-rays Sometimes x-rays (properly called radiographs) are needed as well to help vets visualize your dog’s heart size and shape, as well as any congestion in their lungs caused by their failing ...
This problem can only be diagnosed if all the other problems that cause similar symptoms are ruled out (1), so just limping and walking on the top of the feet could be caused by something else on ...
Microsporum canis is a pathogenic, asexual fungus in the phylum Ascomycota that infects the upper, dead layers of skin on domesticated cats, and occasionally dogs and humans. [ 1 ] [ 2 ] The species has a worldwide distribution.
It was given its variable star designation, BC Canis Minoris, in 1975. [9] It is an aging red giant star currently on the asymptotic giant branch [5] with a stellar classification of M4/5III. [6] It is a semi-regular variable of subtype SRb [4] with measured pulsation periods of 27.7, 143.3 and 208.3 days, and an average visual magnitude of 6. ...
6 Canis Minoris is a star in the equatorial constellation of Canis Minor, located around 570 light years away from the Sun. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of +4.55. [2] This object is moving closer to the Earth with a heliocentric radial velocity of −16.3 km/s. [4]