TrevorW
07-03-2010, 02:20 PM
Target: NGC3572 Cluster associated with nebulosity in Carina
Camera: Canon 350d modified with Astronomik CLS clip filter
Exposure Capture: Maxim
Scope: GSO CF RC200
EFR: f/8
Mount: EQ6 Pro
Exposure Setting: Prime focus, ISO800 ICNR off Daylight WB
Exposures: 18 x 360s taken 6th Match 2010
Seeing: moon not yet risen
Guiding: Orion Starshoot Autoguider using PHD
Focus: Maxim, Bahitov mask
Stacking: DSS 8 x 330s darks no flats, no bias applied
Processing: CS3 levels curves shadow highlights colour balance, Carboni Actions noise reduction, Gradient Exterminator partial crop
Info: Situated in the Carina
Right Ascension (2000.0): 11:10:23.0 (h:m:s)
Declination (2000.0): -60:14:54 (deg:m:s)
m_v: 6.6 (mag)
Dimension: 7.00 (arcmin)
Distance 2300 pc
Size (arc min): 20,0
Cross Identifications: OCL 846, ESO 129-SC1)
Low-dispersion spectroscopy has been obtained for the ringlike nebula which Phelps and Janes (1991) found in the direction of the young open cluster NGC 3572 and suspected as a planetary nebula. Some nearby nebulosities have also been observed. Analyses of these data indicate that all of them, including the NGC 3572 ring, are H II regions. Morphological considerations of the region show that the nearby nebulosities are bright rims which are associated with the H II region BBW 342 and are partly hidden by the obscuring matter lying on this side. The NGC 3572 ring could be of the same nature. However, as the alternative interpretation, it could be a ring nebula (probably a wind-blown bubble) around a massive star (WR/Of star or LBV).
Camera: Canon 350d modified with Astronomik CLS clip filter
Exposure Capture: Maxim
Scope: GSO CF RC200
EFR: f/8
Mount: EQ6 Pro
Exposure Setting: Prime focus, ISO800 ICNR off Daylight WB
Exposures: 18 x 360s taken 6th Match 2010
Seeing: moon not yet risen
Guiding: Orion Starshoot Autoguider using PHD
Focus: Maxim, Bahitov mask
Stacking: DSS 8 x 330s darks no flats, no bias applied
Processing: CS3 levels curves shadow highlights colour balance, Carboni Actions noise reduction, Gradient Exterminator partial crop
Info: Situated in the Carina
Right Ascension (2000.0): 11:10:23.0 (h:m:s)
Declination (2000.0): -60:14:54 (deg:m:s)
m_v: 6.6 (mag)
Dimension: 7.00 (arcmin)
Distance 2300 pc
Size (arc min): 20,0
Cross Identifications: OCL 846, ESO 129-SC1)
Low-dispersion spectroscopy has been obtained for the ringlike nebula which Phelps and Janes (1991) found in the direction of the young open cluster NGC 3572 and suspected as a planetary nebula. Some nearby nebulosities have also been observed. Analyses of these data indicate that all of them, including the NGC 3572 ring, are H II regions. Morphological considerations of the region show that the nearby nebulosities are bright rims which are associated with the H II region BBW 342 and are partly hidden by the obscuring matter lying on this side. The NGC 3572 ring could be of the same nature. However, as the alternative interpretation, it could be a ring nebula (probably a wind-blown bubble) around a massive star (WR/Of star or LBV).