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Strong [O III] and [N II] emission lines in globular clusters from photoionized R Corona Borealis star winds
emission lines globular clusters
2011/1/13
The globular cluster X-ray source CXO J033831.8-352604 in NGC 1399 has recently been found to show strong emission lines of [O III] and [N II] in its optical spectrum in addition to ultraluminous X-ra...
Probing Intermediate Mass Black Holes With Optical Emission Lines from Tidally Disrupted White Dwarfs
Probing Intermediate Mass Black Holes Optical Emission Lines
2011/1/13
We calculate the emission line spectrum produced by the debris released when a white dwarf (WD) is tidally disrupted by an intermediate-mass black hole (IMBH; $M\sim 10^{2}-10^{5}\msun$) and we explor...
The Broad Emission Lines in AGN: Hidden Disk Emission
Broad Emission Lines Hidden Disk Emission
2009/7/9
The Broad Emission Lines in AGN: Hidden Disk Emission。
Double- (and Single-) Peaked Emission Lines as Probes of the Structure of the Outer Accretion Disks in AGN
Peaked Emission Lines Probes Outer Accretion Disks
2009/7/9
Double- (and Single-) Peaked Emission Lines as Probes of the Structure of the Outer Accretion Disks in AGN。
How to accurately estimate BH masses of AGN with double-peaked emission lines
BH masses double-peaked emission lines AGN
2009/7/9
How to accurately estimate BH masses of AGN with double-peaked emission lines。
The properties of optical FeII emission lines of AGN with double-peaked broad emission lines (parte b)
optical FeII emission AGN broad emission lines
2009/7/9
The properties of optical FeII emission lines of AGN with double-peaked broad emission lines (parte b) 。
Chianti-an atomic database for euv emission lines
Chianti-an atomic database euv emission lines
2009/6/4
Chianti-an atomic database for euv emission lines。
Error estimates for emission lines in the hydrogen and helium isosequences
emission lines helium isosequences hydrogen isosequences
2009/6/4
Error estimates for emission lines in the hydrogen and helium isosequences。