Table 1

The Sgr PNe. For the first three objects, stellar magnitude, nebular flux and diameters are derived from the HST images presented here. Data for BoBn 1 are from Wright et al. (2005) but the position was redetermined. Stellar classification is discussed below.

PNlbRight ascensionDeclinationvhel (km s−1)mV (star) (mag)log F(Hα) (erg cm−2 s−1)Diameter (arcsec)Star
(J2000)
He 2-4364.8−22.719 32 06.70−34 12 57.4+13317.25 ± 0.1−11.740.6[WO 4]/[WC 4]
StWr 2-215.2−18.619 14 23.35−32 34 16.6+12919.7 ± 0.1−12.262.7[WO 2]
Wray 16-4236.8−19.819 22 10.63−31 30 38.7+13318.85 ± 0.2−11.551.45[WC 4]/WELS
BoBn 1108.4−76.100 37 16.03−13 42 58.5+174−12.4252
PNlbRight ascensionDeclinationvhel (km s−1)mV (star) (mag)log F(Hα) (erg cm−2 s−1)Diameter (arcsec)Star
(J2000)
He 2-4364.8−22.719 32 06.70−34 12 57.4+13317.25 ± 0.1−11.740.6[WO 4]/[WC 4]
StWr 2-215.2−18.619 14 23.35−32 34 16.6+12919.7 ± 0.1−12.262.7[WO 2]
Wray 16-4236.8−19.819 22 10.63−31 30 38.7+13318.85 ± 0.2−11.551.45[WC 4]/WELS
BoBn 1108.4−76.100 37 16.03−13 42 58.5+174−12.4252
Table 1

The Sgr PNe. For the first three objects, stellar magnitude, nebular flux and diameters are derived from the HST images presented here. Data for BoBn 1 are from Wright et al. (2005) but the position was redetermined. Stellar classification is discussed below.

PNlbRight ascensionDeclinationvhel (km s−1)mV (star) (mag)log F(Hα) (erg cm−2 s−1)Diameter (arcsec)Star
(J2000)
He 2-4364.8−22.719 32 06.70−34 12 57.4+13317.25 ± 0.1−11.740.6[WO 4]/[WC 4]
StWr 2-215.2−18.619 14 23.35−32 34 16.6+12919.7 ± 0.1−12.262.7[WO 2]
Wray 16-4236.8−19.819 22 10.63−31 30 38.7+13318.85 ± 0.2−11.551.45[WC 4]/WELS
BoBn 1108.4−76.100 37 16.03−13 42 58.5+174−12.4252
PNlbRight ascensionDeclinationvhel (km s−1)mV (star) (mag)log F(Hα) (erg cm−2 s−1)Diameter (arcsec)Star
(J2000)
He 2-4364.8−22.719 32 06.70−34 12 57.4+13317.25 ± 0.1−11.740.6[WO 4]/[WC 4]
StWr 2-215.2−18.619 14 23.35−32 34 16.6+12919.7 ± 0.1−12.262.7[WO 2]
Wray 16-4236.8−19.819 22 10.63−31 30 38.7+13318.85 ± 0.2−11.551.45[WC 4]/WELS
BoBn 1108.4−76.100 37 16.03−13 42 58.5+174−12.4252
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