Table 1
General properties of IRAS F11506-3851.
| Properties | Value | References |
|
|
||
| z | 0.01078 | de Vaucouleurs et al. (1991) |
| DL [Mpc] | 46.6a | |
| scale [pc/arcsec] | 221a | |
| log(LIR/L⊙) | 11.30b | Moshir et al. (1992) |
| SFR [M⊙/yr-1] | 34c | Rodríguez-Zaurín et al. (2010) |
| Mdyn [M⊙] | (5 ± 1) ×1010 | Bellocchi et al. (2013) |
| Inclination angle | (37 ± 3)° | Bellocchi et al. (2013) |
| Nuclear Spectral Class. | HII Galaxy | van den Broek et al. (1991) |
Notes.
Luminosity distance and scale using Edward L. Wright Cosmology calculator (Wright 2006).
Infrared luminosity (in solar bolometric luminosity and logarithmic units) defined as LIR = L(8−1000 μm) and calculated using the fluxes in the four IRAS bands as given in Sanders et al. (2003).
Star formation rate computed from the IR luminosity (integrated over the range 8−1000 μm) following 42.
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