
|           | Back to Observing Reports April 15 to 19, 2012 at Ft. Davis NELM 7.0 to 7.8 variable as sky glow
                due to higher than normal solar activity Seeing 3/5 to 4/5 Transparency 4/5   Telescope: 48” f/4.0 reflector Eyepieces:  10 and 6mm
                  ZAO-II, 10mm Delos, 8mm TMB Supermonocentric Images are from the Sloan Digital Sky Survey 
 | 
| 
 08
38
                24.1  +25 45
                15  2.4x0.7’  14.0b 48” (488x)
                - Very nice integral signed galaxy with a very bright
                3:2 elongated core. 
                The east arm is slightly brighter than the west
                arm.  The
                east arm is faint and fairly diffuse and held 100% of
                the time with averted vision.  About 1’ long.  The west arm
                is slightly straighter than the other arm.  The west arm
                stretches about 0.8’ long. 
                A faint round glow appears just south of the
                core. | |
| 
 10
54
                35.1  +56 59
                16  1.6x1.4’  12.9 1.0x0.3’  15.7 48” (488x)
                - NGC 3445 - A bright mottled low surface brightness
                glow with diffuse edges. 
                The primary intent for this object with the 48”
                is to see if I can observe the connector to
                MCG+10-16-24, which I did as a very faint connector
                which goes about 1/3 of the way to the MCG.  MCG+10-16-24 –
                Faint 3:1 elongated diffuse even surface brightness
                glow.  PA =
                90 degrees and 0.4’ long. 
                MAC1054+5700 – Very faint 2:1 even surface
                brightness glow with a bright round very compact core.  PA = 60 and
                0.2’ long.  A
                blazing mag 10.0 star lies 2.1’ NE.  | |
| 
 11
25
                35.2  +54 23
                15  1.1x0.3’  16.6 48” (488x)
                – MCG+9-19-73 - A thin glow with three knots, the
                southern knot is by far the brightest 3:2 elongated
                knot.  The
                middle one is a second brightest knot and is nearly
                stellar.  The
                last, NW knot is the dimmest and is stellar.  Each knot is
                about 20-25” apart. 
                0.8’ long and PA = 150 degrees.  MAC 1125+5423,
                located 2’ due west is a 2:1 bright elongated glow with
                somewhat diffuse edges and a much brighter round core.  PA = 90 and
                0.2’ long.  A
                blazing mag 8.7 star lies just 1’ north of Arp 151. | |
| 
 10
49
                50.1  +32 58
                58  1.8x1.6’  12.0v,  4.2x1.4’  12.6p 48” (488x)
                – Two very mottled glows with quite a few large knots
                and brighter centers. 
                A couple knots detected in the connecting arm. | |
| 
 12
05
                44.7  +31 03
                17  1.4x0.5’  15.3, 1.6x0.5’  15.7 48” (488x)
                - Very cool coat hanger looking group of galaxies.  The hook off
                MCG+5-29-11 is considerably faint, but obvious.  It hooks to
                the west side hooking to the south.  It is brighter
                than the connecting streamer to MCG +5-29-10, which lies
                2.4’ due north.  The
                two mentioned galaxies group forms a coat hanger with
                MCG+5-29-12, despite that there are no bridges to
                MCG+5-29-12.  Very
                cool object in the 48” | |
| 
 11
03
                53.9  +40 51
                00  0.5x0.3’  15.4, 0.4x0.3’  16.5 48” (488 and
                  610x) -
                The penetrator is a 3:1 elongated fairly high surface
                brightness glow with defined edges.  The
                interesting feature is that it has 3 bright knots along
                the middle.  The
                ring galaxy is considerably faint and even surface
                brightness with defined edges. | |
| 
 13
16
                47.3  +14 25
                40  0.9x0.6’  14.8 48” (488x)
                - MCG+3-34-12 easily shows the spiral structure with the
                north arm sharply bends more than the south arm.  The south arm
                is connected to the companion galaxy at the tip and
                doesn’t bend nearly as sharply as the north arm.  The galaxy is
                about 0.5’ due south of the core of MCG+3-34-12.  MCG+3-34-13 is
                a bright round diffuse glow and lies 1.3’ SE of
                MCG+3-34-12. | |
| 
 12
39
                37.6  +16 35
                18  0.5x0.2’  15.9, 0.2x0.1’  17.5, 0.3x0.2’  16.5, 0.2x0.1’  17.0 48” (488 and
                  610x)
                - The east component (consisting of IC 803, MAC
                1239+1635B, D)  is
                a 4:1 elongated glow with three knots.  The middle one
                is the brightest knot. 
                The lone galaxy, NAC 1239+1635C, lies 25” due
                west of the middle knot and is a very bright stellar
                core with a diffuse halo. 
                0’2 across. We didn’t see the extension to the
                SW. | |
| 
 14
35
                08.8  +05 21
                32  1.1x0.7’  13.8 1.3x0.6’  14.5 48” (488 and
                  610x)
                - The original goal of observing this object with the
                48” is to fish out the attached companion that lies
                about 40” SE from the center of NGC 5679B.  The companion
                is a considerably faint very small round glow. | |
| Back to Observing Reports All Observing Reports are copyrighted by Alvin Huey. You can print them for personal use only. | |
| Home
                     About Us       
                Telescopes  
                    Telescope         
                Observing         
                Observing  
                        Dowloadable
                           Observing         
                Links Components Aids Guides Observing Guides Reports |