Jennifer, There are three catalogs that list galactic inclinations cited in this interesting article: http://eo.ucar.edu/staff/dward/sao/dward604project.pdf I haven't looked for any of those catalogs, but I assume they're available. I stumbled across this article when I was looking for a formula to calculate galactic inclination based on observed major and minor axes. Dan Heim ----- Original Message ----- From: "Jennifer Polakis" <m24@xxxxxxx> To: <az-observing@xxxxxxxxxxxxx> Sent: Friday, May 25, 2007 2:17 AM Subject: [AZ-Observing] Re: M101 for the month of May > Chris, > > Another highly detailed photo but do you really think 10x better than your > previous photos with your "old" camera. Definitely 100x better than a > Brownie! > > I wonder to gravitational lensing--when there is a galaxy within the obvious > confines of the nearer galaxy, is it _always_ magnified by the > gravitational lens? Would a camera still pick all of them up if they weren't > magnified by the closer galaxy? > > Jimmy, > As for the inclination of M101 it's actually 17o, and yes, all spiral > galaxies are round. There is a set formula to determine the inclination > based on the length and width + a few degrees for what radio telescopes > pick up beyond that. It's a bit counter-intuitive in that 0 degrees is > perfectly face on and 90 degrees is an edge on. The Andromeda galaxy for > example is inclined 77+degrees. > > Does anyone knows where to find a list of galaxy inclinations, even a small > list like for the M's would be great for a comparison. > > > Chris, > ...The brightest knot in the arms to the upper right of the nuclear region > is NGC5462, an complex blue stellar association with a rim of red hydrogen > around its energetic core. When we add the hydrogen data to this image, the > galaxy dynamics that will become visible here will be simply out of this > world.... > > Actually NGC 5462 is to the left of the nuclear region at about 9:30 with an > even brighter NGC 5461 just below it closer to the nucleus. > > Jenn. > > > > ----- Original Message ----- > From: "Jimmy Ray" <jimmy_ray@xxxxxxx> > To: <az-observing@xxxxxxxxxxxxx> > Sent: Thursday, May 24, 2007 7:49 PM > Subject: [AZ-Observing] Re: M101 for the month of May > > > Hi Chris, > > A great shot! I have it up as my desktop picture so I can admire it for > awhile. > Now for the questions borne of Novice ignorance and curiousity. On your > website there are a couple of statements that I'm pondering over: > > "its inclination is less than 1 degree and is face on to our line of sight." > > How is this actually calculated and/or figured out? Do all spiral galaxies > have a certain degree of "roundness" so any amount of "obliqueness" can be > corrolated into degrees of "tilt" or other? > > "Hordes of faint background galaxies dot this image, most being a leaden > yellow color, dimmed from their great distance through intergalactic dust." > > Is this dust causing the "yellowing" galactic or interstellar dust > collecting around the galaxy itself in the plane of or within the > gravitational field of that galaxy? Or an unrelated dark nebula somewhere > between here and there? And / or is this caused because of the general > "dustiness" of the Universe? > Jimmy Ray > > > Subject: [AZ-Observing] M101 for the month of May > > HI all, > It took all month to image this one, due to clouds, > wind, and giving it lots of exposure time. Anyway, I > think youll like the lastest image of the Pinwheel > galaxy with our newer ST10xme camera. It does 10x > better job on galaxies than the older ST8i with the > same setup and exposures! > http://www.schursastrophotography.com/ccdimagepages/m101-3.html > Comments? > Chris > Take Care, > > Chris > Astro: http://www.schursastrophotography.com > Robotics: http://www.schursastrophotography.com/roboticsmain.html > > > > > > -- > See message header for info on list archives or unsubscribing, and please > send personal replies to the author, not the list. > > -- See message header for info on list archives or unsubscribing, and please send personal replies to the author, not the list.