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11 Camelopardalis
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Star in the constellation Camelopardalis
250px A light curve for BV Camelopardalis, plotted from Hipparcos data
J2000.0
Camelopardalis
05 06 08.45273
+58 58 20.5432
5.08
B3 Ve
−0.080
Be
−6.264
−7.118
4.7543
0.1224
−1.38
6.0 1.2
7.87
4.00 0.35
1766 131 122 commas
17240 560 commas
95 6
25 3
BV Cam 11 Cam +58°804 32343 23734 1622 25001 6193 2480 05062+5900 J05061+5858A
11+Cam
thumb|left|11 Camelopardalis and its reddish companion 12 Camelopardalis
11 Camelopardalis is a single star in the northern circumpolar constellation of Camelopardalis, located around 690 light years away from the Sun as determined by parallax. It has the variable star designation BV Camelopardalis; 11 Camelopardalis is the Flamsteed designation. This object is visible to the naked eye as a faint, blue-white hued star with a baseline apparent visual magnitude of +5.22. It forms a double star with 12 Camelopardalis, which is only 3 arcminutes away.
This is a main sequence Be star with a stellar classification of B3 Ve. John R. Percy et al. discovered that 11 Camelopardalis is a variable star in 1979, and published that finding in 1981. It was given its variable star designation in 1987. Samus et al. (2017) classify it as a Be variable, rather than a Gamma Cassiopeiae type, and it ranges from a peak Hipparcos magnitude of 5.10 down to 5.22. The star is spinning with a projected rotational velocity of 95 km/s, but is being viewed from an extreme pole-on position. Hence it is spinning much more rapidly than indicated. Outbursts of hydrogen emission lines have been observed, as well as rapid changes in hydrogen line profiles. It is 25 million years old with around six times the mass of the Sun.
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Category:Be stars
Category:B-type main-sequence stars
Category:Gamma Cassiopeiae variables
Camelopardalis, BV
Category:Double stars
Category:Camelopardalis
Camelopardalis, 11
Category:Durchmusterung objects
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