The Cycles of Alpha Centauri
2009 ◽
Vol 5
(S264)
◽
pp. 146-149
AbstractThe main AB pair of the nearby Alpha Centauri triple system has one of the most extensive X-ray records of any cosmic object, stretching over three decades. The primary, α Cen A (G2V), is a near twin of the Sun, with a similarly soft (1–2 MK) corona. The secondary, α Cen B (K1V), is more active than the Sun, with a generally harder coronal spectrum. Here, spatially resolved measurements of the pair by Chandra's High Resolution Camera are compared, on a common basis, with previous pointings from ROSAT and XMM-Newton.
2008 ◽
Vol 79
(10)
◽
pp. 10E302
◽
2010 ◽
Vol 81
(10)
◽
pp. 10E312
◽
2004 ◽
Vol 219
◽
pp. 259-263
◽