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Mike JW

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Posts posted by Mike JW

  1. Hi Tony,

    Good to see you are back in action. Excellent wide fov shot with so much on view.  Arp 113 was classified as Ellipticals and Elliptical like galaxies close to and perturbing  spirals. NGC 70 is the spiral and NGC 71 and  68 are presumably the E and E like galaxies but is there any perturbing on the go?

    Mike

    • Thanks 1
  2. This time I visited a couple of targets in Aquarius.

    PCG 221755-013227.  Yeah, I know its just a collection of little fuzz spots. The brightest is mag 18.6 in the centre and the other 3 are mag 19.. They are not a true group. The central gx is about 1.57 Gly and the topmost one is a mere 1.86 Gly.

    1061578974_PCG221755-01322703Nov21_11_59_03.png.6eb836d0702de8c6f4dfaa95d22d488d.png

    PCG 222121+002743 - at first glance I thought they were stars. The two brighter gx are around the mag 17.6.  and are very distant from each other. Top one is 0.860 Gly and the lower one 2.7 Gly. To the left the mag 18.6 is way out there at 3.4 Gly. Look carefully to the right of the lower bright gx, close to and just inside the red line is the fourth group member at mag 18.7 and a mind blowing 7 Gly away.

    144703048_PCG22212100274303Nov21_12_09_52.png.f8fa72487591d971a2106cc41088b19c.png

    Mike

    • Like 2
  3. NGC 561 in Andromeda.  As you can see from the caption details I was not going for 561. I was in fact taking a look at FGC 170 but when the image appeared on the screen, there was this ring galaxy and all sorts of other objects of interest - faint galaxies, quasars and a 3 pairs of stairs surrounding the faint PGC 

    1708936568_FGC17001Nov21_06_29_35.png.fc3e4f16e7d0a27a1671a9c759918ed2.png82756708_FGC17001Nov21_06_31_18.png.a8dab5b49707aaa18723bad0cfc80524.png

    Mike

     

  4. Arp 190 is an interesting object. Dr. Arp classified the pair as galaxies (not S or E) with filaments. However they both appear to be spirals. Arp thought the filament belonged to a third galaxy (the small white spot to the right of the lower galaxy) but this galaxy is likely to be a star in our own neighbourhood. Redshift puts the lower of the pair at about 475 million lyrs away but there is no info on the upper galaxy. The obvious elliptical below the pair has a similar redshift and might there just be a tidal stream between it and lower galaxy of the pair?

    Colour images show the upper spiral as blue and the lower spiral as red.

     

    449417538_Arp19031Oct21_08_56_54.png.43284876c15f4753c945731b5c381e8a.png

    Mike

    • Like 3
  5. Time we had another globular in this thread.

    Pal 2 in Auriga. It is one of the more distant globulars at around the 90,000 lyrs from us. It has a very eccentric orbit and currently is thought to be at its closest to the galactic centre. It is also heading towards at around 133km/s - a bit of a long wait before we get a close up view. The cluster is also partially obscured by lying in the the galactic plane. As it is an old cluster it will have plenty of red stars.

    822513269_Pal231Oct21_06_14_29.thumb.png.5419656ad5ba1df2404e2050dad11a11.png

    607007121_Pal231Oct21_06_14_23.png.a9ccc71c036971148578c7e5b00aa44c.png

    Mike

    • Like 2
  6. EGB -1. I have struggled to find any info on this one, other than it is about 2000lyrs away.

    1326320249_EGB129Oct21_07_33_33.png.e77b427c17615e3c6a5d9dcb64143756.png

    IC 1747 . The CS is mag 15.8. My shot hints at that dark region around the CS.  The thick outer ring has two much brighter sections - bi-polar. Outside of the thick ring I have just started to pick up a fainter fringe. I certainly did not expect to pick up the dark 'spokes' (x 3).

    857323245_IC174729Oct21_07_09_14.png.b3d0ab1a0cbf8fde610d02a23f43a8b5.png

    BV 5-1

    1477919490_BV5-129Oct21_07_32_36.png.b884b53e9bac091ed076c565d931dbb9.png

    and here is another BV in Cassiopeia 

    BV 5-2 - another weird PN. Nice image - Böhm-Vitense 5-2 (BV 5-2, Sh 2-179) PN G121.6+00.0 photo - jshuder photos at pbase.com

    1009467910_BV5-229Oct21_07_29_03.png.d0077fb1fdb77b8311a24db3511b4ece.png

    Mike

    • Like 4
  7. Hi Bill,

    At last I got to take a look at 29P. I was amazed at how extensive the halo has become. It also appears to have a double nucleus -  which I assume is a star it is about to crash into!!!

    1808517306_Comet29P30Oct21_11_37_58.png.f951e7669fbbf9858fd5f0b70005a80a.png

    Mike

    PS and here is a better shot 24hrs later. The nucleus looks elongated, inner and outer halo. Also there is a sliver of brightness coming off the nucleus (to the right and up)

    896803481_COMET29P31Oct21_06_02_54.png.9efcbea88e4ae7bd16d35508201c62b9.png
     

    • Like 2
  8. Simeiz 22 (Sh 2 -188) is an intriguing object. Why just an arc?, why filaments?.

    See Sh2-188 Nebula (iac.es)  for the full picture. Sure enough there is more going on than just an arc.

    See 901405.pdf;sequence=1 (herts.ac.uk) for a model of how its structure has come about. Briefly put the model suggestion a triple wind hypothesis.  Initially there was the Asymptotic Giant Branch (AGM) wind. This is the slow solar wind that a star in the giant red stage is sending out. It would appear that this wind as it slammed into the Inter Stella Medium caused the bright arc (and tail) that we see. At this stage a PN had not formed. Next as the star collapsed the fast stellar wind blasted outward forming a ring structure (see the first link) as the two winds interacted. However the star is moving quite fast through the  inter stella medium (ISM) - 125+/-Kms towards the bright arc and this third wind along with the other two winds has given rise to the observed structure.  The bright arc is a result of the high velocity of the central star in the direction of this bright arc. The star is displaced from the geometric centre and its high velocity causing thin shock compressed  filaments concentric to the bright arc. Sh 2-188 is one of the largest PN known, about 8.5 lyrs across.

    1211059886_Simeiz2229Oct21_06_59_22.png.0315461bb300fab8b3e71541c9236962.png

    Mike

     

     

    • Like 5
  9. Hi,

    A few thoughts.

    No need to get a focal reducer as your scope is F5.

    Stacking in Sharpcap - I think you need to buy the SharpCap Pro version to do stacking. Personally I find sharpcap way to complicated for my EEVA observing - never had success with it but others do well with it.

    Cheap! - you get what you pay for (whether for cameras, scopes, mounts)

    Mono cameras are more sensitive than colour cameras.  Altair GPCAM2 290M Mono Guide Imaging EAA Camera would probably get you started. I tried one of these but did not get on with the Altair software or Sharpcap - I am not particularly software minded!

    Hopefully you have looked through the EEVA section to see what folk are doing/scopes being used.

    Jupiter/Albireo - OK you were trying things out but you get better views visually with your scope then messing about with a camera on those objects.

    Mike

    • Thanks 1
  10. Hi Martin,

    Always enjoy your colour views of clusters. Surprised me just how many yellow (orange) stars there are in this one - function of the clusters age?  I shall note this gem for a visual look at the "diamonds sparkling away against the black background" with the 15 (wish I still had the 20!).

    Below is the Aladin/SDSS9 view.

    image.png.0abff3c1897f2deda59266b241e40812.png

    Mike

    • Like 1
  11. Hi David,

    Excellent read and so informative, highlighting just what can be observed using the EAA technique. I fancy the answer to why do the arms curve back to the centre could be due to the angle of view?

    Mike

  12. Hi Martin,

    I have just had a very enjoyable read of the articles. I viewed these Arps a year ago but did not seek out any further information - glad you did. Minkowski Object  - how interesting and  re-looking at my original shot I should have pondered what was happening. Also I had not picked up that NGC 541 had at some point interacted with NGC 547 and hence the tidal stream between the two galaxies. Below is rather a messy shot (lots of dust bunnies had to be lost!) using the C11 from last year. If I get a chance I will point the 15 at it and see if I can get more of the tidal stream/cleaner view.

    678302075_Arp13317Oct21_10_00_47.png.366edcd0ba2c72d91f12abd92a802c09.png

    Mike

     

    • Like 3
  13. and here is four more from Aquarius.

    SHK 334                                                                                                                   SHK 302 - there is meant to be 9 in the group but I cannot locate it! They are 1.1/1.2 billion lyrs away.

    315324543_SHK33413Oct21_17_48_04.png.47fa77c86ed8cf8fe1f24be46ead44ba.png758352265_SHK30213Oct21_18_03_26.png.49956c2f9d2f28350313fcf0c0fc97c4.png

    SHK 301 - tonight's mystery! Absolutely nothing there. NED locates 301 to           SHK 303 - So close to the bright star that I missed it at first.

    the same place but shows no galaxy group!!!!

    91546155_SHK30113Oct21_17_59_21.png.83064190a657c5e07ca4dbdf20a5c415.png762892861_SHK30313Oct21_18_09_30.png.b0f264c3ac9e2a65f902250d5b14baf5.png

    • Like 3
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