HD 24479 [SEP] constellation
HD 24479
HD 24479 (or H Camelopardalis), is a single star located in the constellation Camelopardalis. It is also known as HR 1204. The star is visible to the naked eye with an apparent visual magnitude of 4.95. Based upon an annual parallax shift of as seen from Earth's orbit, it is located around 360 light years from the Sun.
In 1932, HD 24479 was identified as a Be star by Olin C. Wilson at the Mount Wilson Observatory. In 1969, Cowley et al.
Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-21-42. During World War II, various changes were made in the makeup of the 55th CA. The 55th CA (