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| | Phi And (Site not responding. Last check: 2007-10-11) |
 | | Separately, the brighter, Phi And A, seems to be a fifth magnitude (4.54) B6 subgiant, while the fainter, Phi And B, is a sixth magnitude (5.55) B9 dwarf (the magnitudes uncertain and scaled to fit to the measure of the combined stars). |
 | | Phi And A -- like Gamma Cas and Zeta Tauri -- is a "B- emission" ("Be") type star, one with a circulating circumstellar disk that radiates emission lines (the origins of which are not at all clear). |
 | | Phi And A's observed rotation speed is relatively low, however, only 81 kilometers per second, implying that the rotation axis is rather well tilted toward us (such speeds being projections against the sky and therefore lower limits). |
| www.astro.uiuc.edu /~kaler/sow/phiand.html (554 words) |
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