Uwe Glahn
May 20th, 2013, 04:54 PM
Last month I had the opportunity to use the powerful 2400 square inches of Jimi's Barbella, thanks Jimi for this "cosmic adventure" :)
One of the target was the famous Ringnebula Messier 57 but not with a "normal" filter to enhance the emissions of the nebula itself. We use a "central star filter" which works opposing all these famous filters. Reiner Vogel measured some spectra of this filter (aborptions (http://www.reinervogel.net/Filter/spectra/Astroelectronic_ZS_a_UG.jpg) and transmission (http://www.reinervogel.net/Filter/spectra/Astroelectronic_ZS_t_UG.jpg)) The goal is to disable the nebula which outshines faint stars. Famous target is for example the PN NGC 6210.
Without the filter both central stars were visible easily and with direct vision. Magnification was around 814x (Jimi correct me when my memory is wrong), Seeing was average. When we put the filter in, the filter effect on the two central stars was not prominent. But at the outer ring areas the filter showed a very good response. The nebula was visible just very faint and some stars glimpsed out very well. I tried to sketch the roughly positions of the stars (see sketch below) at the few minutes on the ladder and detected 7 stars. All stars but the star at 11.30 (CS middle, north/up 12.00) were easily visible. I don't noticed which was direct/averted vision. Some more stars should be visible when the seeing is better and you more time on the ladder.
My reworking and investigations were much harder than I expected. Perhaps we were the first observers how saw this stars visually. To bring out the exact position was also very hard, even on the HST images some stars were totally out-shined. I tried to compile some very good images. But it is nearly impossible to get the visual positions and relative magnitudes because of the different spectra sensitivities. I think an photographer or a Mallincam with a CS filter has to imagine the PN to get a good card of these stars.
It would be a very exciting project to get these stars, not only within M57 and not only with 2400 square inches
sketch: 48", 814x, CS filter, seeing III, NELM 7m+
666
-----------------------------------------------------
HST color image
- stars seen are labeled with solid line
- stars which could be in reach with broken line
667
-----------------------------------------------------
HST WFPC2 with 469N (He II) filter (2MASS on)
668
-----------------------------------------------------
HST WFPC2 with 547M (strömgen y) filter (2MASS on)
669
-----------------------------------------------------------
amateur image - Spiegelteam - Capella Observatory/Crete
24"; LRGB (Ha/[OIII]/[OIII]), Wendel, Binnewies, Pöpsel
RGB imgage (http://www.spiegelteam.de/m57.htm)
-----------------------------------------------------------
UCLA Infrared Laboratory
infrared image (http://irlab.astro.ucla.edu/images/gallery/flitecam/RingNebula_M57_J.jpg)
One of the target was the famous Ringnebula Messier 57 but not with a "normal" filter to enhance the emissions of the nebula itself. We use a "central star filter" which works opposing all these famous filters. Reiner Vogel measured some spectra of this filter (aborptions (http://www.reinervogel.net/Filter/spectra/Astroelectronic_ZS_a_UG.jpg) and transmission (http://www.reinervogel.net/Filter/spectra/Astroelectronic_ZS_t_UG.jpg)) The goal is to disable the nebula which outshines faint stars. Famous target is for example the PN NGC 6210.
Without the filter both central stars were visible easily and with direct vision. Magnification was around 814x (Jimi correct me when my memory is wrong), Seeing was average. When we put the filter in, the filter effect on the two central stars was not prominent. But at the outer ring areas the filter showed a very good response. The nebula was visible just very faint and some stars glimpsed out very well. I tried to sketch the roughly positions of the stars (see sketch below) at the few minutes on the ladder and detected 7 stars. All stars but the star at 11.30 (CS middle, north/up 12.00) were easily visible. I don't noticed which was direct/averted vision. Some more stars should be visible when the seeing is better and you more time on the ladder.
My reworking and investigations were much harder than I expected. Perhaps we were the first observers how saw this stars visually. To bring out the exact position was also very hard, even on the HST images some stars were totally out-shined. I tried to compile some very good images. But it is nearly impossible to get the visual positions and relative magnitudes because of the different spectra sensitivities. I think an photographer or a Mallincam with a CS filter has to imagine the PN to get a good card of these stars.
It would be a very exciting project to get these stars, not only within M57 and not only with 2400 square inches
sketch: 48", 814x, CS filter, seeing III, NELM 7m+
666
-----------------------------------------------------
HST color image
- stars seen are labeled with solid line
- stars which could be in reach with broken line
667
-----------------------------------------------------
HST WFPC2 with 469N (He II) filter (2MASS on)
668
-----------------------------------------------------
HST WFPC2 with 547M (strömgen y) filter (2MASS on)
669
-----------------------------------------------------------
amateur image - Spiegelteam - Capella Observatory/Crete
24"; LRGB (Ha/[OIII]/[OIII]), Wendel, Binnewies, Pöpsel
RGB imgage (http://www.spiegelteam.de/m57.htm)
-----------------------------------------------------------
UCLA Infrared Laboratory
infrared image (http://irlab.astro.ucla.edu/images/gallery/flitecam/RingNebula_M57_J.jpg)