Fleming's Triangular Wisp
2016/11/12. One day before the brightest Moon in over half a century, I decided to photograph the fainter bits of a bright(ish) supernova remnant. The Veil Nebula consists of three, maybe four, primary regions: the bright arcs to the east and west (see previous pages) and a large area of much fainter stellar wreckage in the middle (see below!). "Cobwebs" trail off to the south. Right between the two brightest arcs is an area usually called "Pickering's Triangle." By right it should be called "Fleming's Triangular Wisp."
Williamina Fleming's Triangular Wisp
7x900s H-a + 7x900s O-iii (3h 30m)
sum of all exposures used as luminance,
O-iii mapped to blue and green, H-a to red.
TMB92SS @ F4.4, ST2000XM, Baader filters.
Why, yes, you may click for a bigger view.
From the Open Collections Program at Harvard University:
[my addenda appear in square brackets]
Williamina Paton Stevens Fleming [aka "Mina Stevens"] was born in Dundee, Scotland, on May 15, 1857. Her talent in school was obvious from an early age, and at age 14 she began teaching in the Dundee public schools. In 1877 she married James [Orr] Fleming [of Glasgow], and a year later the couple immigrated to Boston to start a new life in America. In 1879, when she was pregnant with her first child, James left her and their unborn son. 
Only 23 years old and a single mother, Fleming found employment as the housekeeper for Edward [Charles] Pickering, a professor of astronomy at Harvard and the director of the Harvard College Observatory. Irritated by the poor work done by his male employees at the observatory, Pickering reportedly declared that his maid could do a better job, and shortly thereafter, in 1881, he hired Fleming to do some clerical work and mathematical calculations at the Observatory. 
Fleming quickly proved Pickering right by developing a new system to classify stars according to their spectra... Thanks to her new classification system, which became known as the "Pickering-Fleming System," Fleming cataloged over 10,000 stars within the next nine years. In 1890, she published her findings in the Draper Catalogue of Stellar Spectra.
Pickering eventually put Fleming in charge of editing all studies published by the Harvard Observatory and allowed her to hire dozens of young women to support her expanding stellar exploration efforts. One of these young women was Henrietta Swan Leavitt, who later discovered how to measure the universe. In 1898, the Harvard Corporation appointed Fleming to be the curator of astronomical photographs at the Harvard College Observatory, making her the first woman to hold this important position. 
During the course of her [32 year] career, Fleming discovered 10 novae, 52 nebulae, and 310 variable stars...  Recognizing her contributions to the discipline, in 1906 the Royal Astronomical Society elected Fleming to its organization, the first time that prestigious body admitted an American woman. In 1910, she reached the pinnacle of her career by discovering white dwarfs, which are very hot and dense stars that are white in color. On May 21, 1911, Fleming died of pneumonia in Boston, Massachusetts.
Williamina Fleming standing at center, c. 1891.
Note variable star plot to viewer's left (Beta Auigae, an eclipsing binary, from Dec 1889).
The other plot may depict the light curve of an eclipsing binary during a single minimum.
Harvard College Observatory Director Edward C. Pickering is in back.
Among other names in the photo: Annie Jump Cannon (front center), and
Henrietta Swan Leavitt (rear left, with magnifying glass).
- In her naturalization petition, Williamina says she arrived in America on December 3, 1878, in New York. In the 1900 census, she says "1884." Wait! See below, she who came in 1884 is the astronomer's niece.
- Was Fleming a single mother or pregnant when she went to work for Pickering? Her son was born on October 6, 1879, and she named him Edward Pickering Fleming, after her employer. Yet Williamina listed his birthplace as Dundee, Scotland, and he was naturalized as a U.S. citizen on the same date as his mother, January 12, 1904. Williamina sent Edward to MIT. He made a career as a chemist and metallurgist in Salt Lake City. Throughout his life, Edward P. Fleming listed his place of birth as Dundee.
- Should be, "She hired dozens of young women to conduct the work of the observatory, prepare reports, make revisions, do calculations..." etc. She lamented that very little time, opportunity, or resources were available to pursue original work.
- Such ennumerations caught the attention of the contemporary press, but they happened in the course of other research. Her real contributions were epic, Sisyphusian, and Herculean: the Draper Catalog and the spectral classification techniques that enabled it, the observatory's year-in year-out surveys, endless plate-cataloging, and staffing. Williamina had a key role (perhaps the key role) in managing "the trenches" of daily work at the Harvard headquarters as well significant rolls in keeping remote stations in western Massachusetts and Peru organized and efficient.
In 1890, while examining a plate made in 1888, Fleming discovered the Horsehead Nebula in Orion. I do hereby and henceforth resolve to call it "Fleming's Pony."
In 1904, Fleming noticed the tangle of filaments in the center of the Veil Nebula in Cygnus. The director's name was attached to the discovery, perhaps by custom, possibly with Fleming's approval (she'd named her son after the director after all). Hence the common name for this nebula: "Pickering's Triangle."
After Williamina Fleming took charge of staffing the observatory with computers, she hired women exclusively (or almost exclusively). The computing department came to be called "Pickering's Harem." Women were meticulous and reliable, she believed, anxious to find meaningful work, and generally grateful and loyal when they got it. It is also true that they worked for less money. By 1900, Fleming's salary had approximately tripled from $10.50/week to $1,500 per year (she says that men in similar jobs were paid $2,500). She was hired to work 7 hours a day for 6 days a week but generally worked from around 9AM to around 6PM, or about 9 hours per day. All was not work: evenings and Sundays she often attended plays at the Castle Square Theater with Annie Jump Cannon and a few of the other "computers."
By 1900, Fleming had hired an Irish servant, Marie Hegarty, to help keep up with her home (267 Upland Avenue, in a warren of residential streets a short walk north from the observatory). Before 1910, Mary McMurray, a Scot, had taken Marie's place, and Williamina's mother Mary Stevens (77) who immigrated in 1887, had joined the household at 57 Concord Avenue, on or adjacent the Observatory grounds. And apparently just to frustrate inquiring minds, Williamina's niece Williamina Fleming (18 years younger than Williamina Fleming), a stenographer who had come to America in 1884, lived there, too. The older Williamina, our Williamina, is shown in the 1910 census as widowed, the younger single. So how is it that they are both "Fleming"?
Let's talk about something simpler
2016/12/06 I interrupt this page to note that Dava Sobel has just released The Glass Universe about Fleming (and the other computers, of course). I'm sure it's a good book. But damn. She even uses the same photo of Pickering's computers on the cover (actually, one made moments before or after). No, I didn't have "plans" or even intend to do more with this, but still, bird-dogging others' books gets old. Harrumph! Back to November.
My photo of Fleming's Triangular Wisp, is a bi-color narrow-band composite. I took 1h45m of data in the light of doubly ionized oxygen (O-iii) and another 1h45m in the light of excited hydrogen (hydrogen-alpha). Then I wasted hours working with a classic green-synthesis version: take the mean of the blue and red signal and use that as green; combine all three channels to make a color image. No matter what I did, the nebula was unclear, fuzzed out, no damn good. I decided to call it a night and went to shower. And there realized that in this case the mean of the two signals was manufacturing not just a green surrogate intensity but entirely fictional light-producing regions. Here, the H-a and O-iii images look very different. Entirely distinct regions light up in each wavelength, not the same regions at different intensities. So I dried off, put on my robe, and tried it again without a synthetic green channel. Instead, I used the O-iii signal for both blue and green while increasing the weight of red (hydrogen-alpha) to compensate for the "extra vote" given to O-iii. The result is as you see.
My deep-sky photos are made with a variety of sensors and optics. Deepest images usually come from a SBIG ST2000XM CCD behind a 10-inch Astro-Tech Ritchey-Chretien carried on an Astro-Physics Mach1GTO. The CCD is equipped with a CFW-10 loaded with Baader wide- and narrow-band filters. Camera control and guiding are handled by Maxim DL 5.12. A Canon 6D and a modded 50D find themselves mounted behind an Orion 10" F4 Newtonian or a 92mm Thomas Back refractor or a tiny but mighty AT65EDQ refractor, sometimes with Backyard EOS in control and PHD Guide keeping things on target. Really widefield photos are often made using the 6D and various camera lenses and an iOptron Skytracker mount. PixInsight does most of the heavy lifting in post-processing — alignment, stacking, gradient removal, noise-reduction, transfer function modification, color calibration, and deconvolution. Photoshop along with Focus Magic and a handful of other plugins get their licks in, too, especially when polishing for the web.
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