Parameter . | Fiducial value . |
---|---|
Stand-off radius for the bow shock | |$R_{\rm SO}=3\times 10^{11}\, {\rm cm}$| |
Zenith angle between the orbital angular momentum direction of the star and the AGN disc | θ* = 80° |
AGN density | ρAGN = 3 × 10−10 g cm−3 |
Scale height of the AGN disc | HAGN = 1012 cm |
Orbital period of the star | |$P_{\rm orb}=20\, {\rm h}$| |
SMBH mass | |$M_{\rm SMBH}=10^6\, {{\rm M}_\odot }$| |
Orbital eccentricity of the star | e = 0 |
Power-law slope for the vertical AGN gas density profile | n = 6 |
Parameter . | Fiducial value . |
---|---|
Stand-off radius for the bow shock | |$R_{\rm SO}=3\times 10^{11}\, {\rm cm}$| |
Zenith angle between the orbital angular momentum direction of the star and the AGN disc | θ* = 80° |
AGN density | ρAGN = 3 × 10−10 g cm−3 |
Scale height of the AGN disc | HAGN = 1012 cm |
Orbital period of the star | |$P_{\rm orb}=20\, {\rm h}$| |
SMBH mass | |$M_{\rm SMBH}=10^6\, {{\rm M}_\odot }$| |
Orbital eccentricity of the star | e = 0 |
Power-law slope for the vertical AGN gas density profile | n = 6 |
Parameter . | Fiducial value . |
---|---|
Stand-off radius for the bow shock | |$R_{\rm SO}=3\times 10^{11}\, {\rm cm}$| |
Zenith angle between the orbital angular momentum direction of the star and the AGN disc | θ* = 80° |
AGN density | ρAGN = 3 × 10−10 g cm−3 |
Scale height of the AGN disc | HAGN = 1012 cm |
Orbital period of the star | |$P_{\rm orb}=20\, {\rm h}$| |
SMBH mass | |$M_{\rm SMBH}=10^6\, {{\rm M}_\odot }$| |
Orbital eccentricity of the star | e = 0 |
Power-law slope for the vertical AGN gas density profile | n = 6 |
Parameter . | Fiducial value . |
---|---|
Stand-off radius for the bow shock | |$R_{\rm SO}=3\times 10^{11}\, {\rm cm}$| |
Zenith angle between the orbital angular momentum direction of the star and the AGN disc | θ* = 80° |
AGN density | ρAGN = 3 × 10−10 g cm−3 |
Scale height of the AGN disc | HAGN = 1012 cm |
Orbital period of the star | |$P_{\rm orb}=20\, {\rm h}$| |
SMBH mass | |$M_{\rm SMBH}=10^6\, {{\rm M}_\odot }$| |
Orbital eccentricity of the star | e = 0 |
Power-law slope for the vertical AGN gas density profile | n = 6 |
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