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Did you spend the night in your truck? Did you find a hidden dirtroad to camp out on, or what did you do up there when the night ran out and you wanted to rest up a bit?
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Great sketch of M51 and its companion there, Akarsh! I wonder what was the highest magnification you employed in your study? Here is my CN post where I mention the three to four brightest H-II/SFRs and OB associations visible inside the spiral with a 10-inch. It's really tough to observe them and the whole galaxy without it taking all night...especially when you have that big a telescope under that dark of skies! I mean, I can tell from your sketch that you hit the big picture. Maybe next time you'll be able to hit the "little picture" details.
"[Sh 2-54] I'm usually not a nebula guy, but this is what showed up as well-placed on my list. "A modestly bright, roundish piece of nebulosity easily observed with DGM NPB filter."Not usually a nebula guy? Hmm, that's the complete opposite of me! I've seen what you saw with my 130mm reflector, 59x, and a NPB filter. From what I understand, Sharpless cataloged the large, faint nebulosity while Simiez Observatory only picked out the small, bright nebula you and I saw. I'd have to do more digging to give you more than that.
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16x80 finder (8/10/91): very large, very faint emission haze (Sh 2-54 = Gum 84) surrounds a very large group of stars, improves with UHC filter. The Eagle Nebula was very prominent in the field to the south. On the north side of this large HII region is a small brighter knot = Simeis 3-132 that was visible in the 17.5" at 64x using a UHC filter as a moderately bright, 3'x2.5' glow, slightly elongated N-S. The eastern side of this HII knot has a sharper, linear border. Also viewed at 220x unfiltered and a group of a half dozen mag 12-13 stars extended N-S in a string are superimposed near the eastern boundary. This obscure, but relatively easy nebula is located 30' N of open cluster NGC 6604 on the north end of Sh 2-54.
On Jul 9, 2022, at 7:40 AM, Scott Harrington <sn4...@gmail.com> wrote:
Before Stewart Sharpless published his 1953 list of 142 emission nebulae found on POSS plates between 17h RA and 0h RA, Grigory Shajn and Vera Gaze published three major lists containing nearly 400 emission nebulae that they had found between 0h RA and 24h RA on plates taken at the Simeis Observatory. Shajn and Gaze tried to cross-reference as many of the nebulae as they could, but believed that at the time of their Third List of Diffuse Nebulae publication in 1952, they were the first to discover 279 nebulae (which they designated with an “S”). Apparently Sharpless knew of the discoveries at the Simeis Observatory prior to the publication of his 1953 catalog because he tried to cross-reference as many of his finds with those. That’s why in his “Notes” column he lists alternate NGC, IC, and S designations. Thus, he knew he was the original discoverer of less than half of the 142 he listed.
However, nowadays, few nebulae are called by their Simeis designation due to the effects of the Cold War. This is truly sad when you consider that Vera Gaze died in 1954 a few months short of her 55th birthday and Grigory Shajn died in 1956 at the age of 64. Just before Gaze died, though, their Fourth List of Diffuse Nebulae (their last one) was published, bringing the grand total of nebulae they believed they were the first to discover to 292*. Of course, I suspect (but haven’t taken the time to prove it) that a few of what they thought were original finds when their last list was published were actually published by Sharpless a year prior.
The supernova remnant Simeis 147 might just be their most famous find. Oddly, there are a few of their finds that carry their crude catalog designation when they should instead carry their original discovery designation. For example, Simeis 3-210, 3-206, and 3-204 is a far southern part of the Veil Nebula that should actually be known as Simeis 243/45/49 even though it was simply labeled Simeis 3-210 on page 30 of Howard Banich’s Sep ’21 S&T article. Also in Howard’s article, he gives Fleming’s Triangle the designation Simeis 3-188, when it should instead be Simeis 227/28/29. That’s a "mistake" that might have been carried over from Steve Gottlieb’s online piece “Dissecting the Veil Nebula”. Interestingly, Sue French does call it Simeis 229 in her Oct ‘03 S&T article “On the Wings of the Swan”.
Certainly not this month, but maybe next month I’ll have to time to put together a master list where I show which Sharpless emission nebulae (or H-II regions as he preferred to call them in his 1959 catalog) carry a Simeis original discovery designation so that we can start using them again and give credit where credit is due. None of it will be easy, though.
*In the Fourth List of Diffuse Nebulae, they reached S 301, but noted that two of their original finds in the first list along with five in the second list had actually been discovered prior. They also noted that S 31 and S 121 didn’t truly exist.
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