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- W1973432807 abstract "We report [O iii] λ5007 and [N ii] λ6583 emission from a globular cluster harboring the ultraluminous X-ray source CXOJ033831.8 − 352604 in the Fornax elliptical galaxy NGC 1399. No accompanying Balmer emission lines are present in the spectrum. One possibility is that the forbidden lines emanate from X-ray-illuminated debris of a star that has been tidally disrupted by an intermediate-mass black hole, with this debris also feeding the black hole leading to the observed X-ray emission. The line strengths indicate that the minimum size of the emitting region is ∼1015 cm, and if the 70 km s−1 half-widths of the emission lines represent rotation around the black hole, a minimum black hole mass of 1000 M☉ is implied. The non-detection of Hα and Hβ emission lines suggests a white dwarf star was disrupted, although the presence of strong nitrogen emission is somewhat of a mystery." @default.
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- W1973432807 date "2010-02-24" @default.
- W1973432807 modified "2023-09-27" @default.
- W1973432807 title "EVIDENCE FOR A STELLAR DISRUPTION BY AN INTERMEDIATE-MASS BLACK HOLE IN AN EXTRAGALACTIC GLOBULAR CLUSTER" @default.
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- W1973432807 doi "https://doi.org/10.1088/2041-8205/712/1/l1" @default.
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