# Table 5 - Inferred physical properties for the # Marino et al (2010) LGG galaxy sample #____________________________________________________________________ # Galaxy ID Morph T theta M_B log Mgal log SFR_o b Type #____________________________________________________________________ _______________________________ LGG 93 ______________________________ NGC 1249 SBc 6.0 -1.02 -19.57 10.53 0.453 1.07 NGC 1311 SBm 8.8 -1.07 -18.30 9.69 0.009 2.67 IC 1933 Sc 6.1 -1.16 -18.66 10.16 0.226 1.52 IC 1954 SBb 3.2 -0.96 -19.72 10.93 0.423 0.40 IC 1959 SBd 8.4 -1.29 -18.21 9.70 -0.065 2.19 _______________________________ LGG 127 _____________________________ NGC 1744 SBcd 6.7 -1.18 -20.24 10.72 0.626 1.04 NGC 1792 SBbc 4.0 -0.24 -22.42 11.91 1.376 0.38 NGC 1800 Sd 8.2 -1.22 -18.78 9.95 0.090 1.77 NGC 1808 SABa 1.2 -0.36 -22.21 12.16 1.035 0.10 NGC 1827 SABc 5.9 -0.22 -19.96 10.70 0.886 1.97 ESO305-009 SBd 8.0 -1.31 -18.39 9.82 -0.022 1.85 ESO305-017 IB 9.9 -1.29 -17.14 9.10 -0.504 3.25 ESO362-011 Sbc 4.2 -2.85 -17.74 10.01 -1.000 0.13 ESO362-019 SBm 8.9 -1.31 -17.72 9.45 -0.314 2.24 ________________________________ LGG 225 ____________________________ NGC 3370 Sc 5.1 -1.24 -19.76 10.72 0.207 0.40 NGC 3443 Scd 6.6 -1.18 -17.26 9.54 -0.208 2.32 NGC 3447 Sm 8.8 -1.40 -17.31 9.29 -0.014 6.33 NGC 3447A IB 9.9 -1.76 -15.15 8.30 -0.768 11.0 NGC 3454 SBc 5.5 -0.62 -19.08 10.39 -0.209 0.32 NGC 3455 SABb 3.1 -0.73 -18.31 10.37 0.434 1.48 NGC 3501 Sc 5.9 -0.78 -18.99 10.31 -0.142 0.45 NGC 3507 SBb 3.1 -1.07 -20.10 11.09 0.422 0.28 UGC 6022 I 9.9 -1.31 -14.87 8.19 -1.127 6.27 UGC 6035 IB 9.9 -1.27 -16.48 8.83 -0.695 3.82 UGC 6083 Sbc 4.1 -0.82 -17.39 9.88 -0.722 0.32 UGC 6112 Scd 7.4 -1.04 -17.49 9.54 -0.248 2.12 UGC 6171 IB 9.9 -1.60 -16.36 8.78 -0.847 3.02 #____________________________________________________________________ Notes: Morphological-type classification from the Marino et al (2010) compilation; spectral slope theta from (FUV-NUV) color as theta = -[2+0.4(FUV-NUV)/log(1520/2300)]; absolute B magnitude M_B from B_T from RC3 (de Vaucouleurs et al. 1991), except UGC6022, which is from UGC (Nilson 1973), after correction for reddening (see footnote 15) and distance, the latter derived from the mean redshift of the parent group, assuming a pure Hubble flow with H_o=75km/s/Mpc; galaxy stellar mass in M_sun from M/L_B, according to Buzzoni (2005); SFR in M_sun/yr from the dereddened NUV flux, according to footnote 16; birthrate b assumes a current galaxy age of 13 Gyr.