Our 5 ks { \it Chandra } ACIS-S observation of the globular cluster NGC 6652 detected 7 X-ray sources , 3 of which are previously unidentified .
This cluster hosts a well-known bright low-mass X-ray binary , source A ( or XB 1832-330 ) .
Source B shows unusual rapid flaring variability , with an average L _ { X } ( 0.5-10 keV ) \sim 2 \times 10 ^ { 34 } ergs/s , but with minutes-long flares up to L _ { X } = 9 \times 10 ^ { 34 } ergs/s .
Its spectrum can be fit by an absorbed power-law of photon index \Gamma \sim 1.24 , and hardens as the countrate decreases .
This suggests that part or all of the variation might be due to obscuration by the rim of a highly inclined accretion disk .
Sources C and D , with L _ { X } \sim 10 ^ { 33 } ergs/s , have soft and unusual spectra .
Source C requires a very soft component , with a spectrum peaking at 0.5 keV , which might be the hot polar cap of a magnetically accreting polar cataclysmic variable .
Source D shows a soft spectrum ( fit by a power-law of photon index \sim 2.3 ) with marginal evidence for an emission line around 1 keV ; its nature is unclear .
The faint new sources E , F , and G have luminosities of 1-2 \times 10 ^ { 32 } ergs/s , if associated with the cluster ( which is likely ) .
E and F have relatively hard spectra ( consistent with power-laws with photon index \sim 1.5 ) .
G lacks soft photons , suggesting absorption with N _ { H } > 10 ^ { 22 } cm ^ { -2 } .