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Captured 3 Nov 20, 20:57 hrs ET, Springfield, VA, USA. Bortle 8 skies, MallinCam DS10c camera, 10 inch SCT f6, exposure 60 sec, gain 60, bin 1, stack 10, LeNhance filter.
Clouds: clear
Seeing: 30
Transparency: 30
FOV: 37 x 28 arcmin
Moon phase: 94%
Apparent magnitude: +xx
Size: 20 arcmin
Surface brightness: xx magnitudes per square arcmin
Appearance: Low contrast, roughly circular red emission nebula in a dim starfield. The open cluster Stock 18 is centered at the nebula.
REF: Sharpless 170 and the surrounding interstellar medium. Roger, McCutcheon, Purton, and Dewdney.
Astronomy and Astrophysics, v.425, p.553-567 (Oct 2004).
"Sharpless 170 is a diffuse HII region (in Cas) ionized by a single main sequence O-star located near the periphery of a small dense molecular cloud at a distance of ∼2 kpc...From the thermal continuum emission we estimate the mass of ionized gas at ∼350 M☉ within a radius of ∼7 pc. The HI (λ21 cm) and far-infrared observations show an extended low-density atomic component, of ∼1000 M☉, within an irregular boundary surrounding the ionized gas of mean radius ∼10 pc. Mean densities in the HI and HII are similar, in the range 9-16 nucleons cm-3. CO emission shows a molecular cloud of ∼1150 M☉ within an area 6 pc × 4 pc with densities ∼2000 nucleons cm-3. A compact infrared component coincides with the cloud. The exciting star is located on the near side of the cloud, just inside the southern periphery.
Sh170 is an example of a young HII region with the ionized gas, seen in Hα emission, streaming outward in the manner of a ``champagne flow''. Although the observed velocities of the HI are close to the mean velocity of the CO cloud, the morphology of the associated atomic hydrogen closely resembles that seen in the surrounds of other young HII regions which show clear evidence of expansion of their HI.
We propose that much of the HI is a diffuse dissociation zone beyond the ionization front, in directions from the star within a wide annulus, approximately transverse to the line-of-sight, between the dense photon-bounded region on the far side of the star and the density-bounded ionized flow region on the near side. In this view, much of the associated atomic gas, like the ionized gas, has been eroded from the molecular cloud in a small fraction (≤10%) of the star's main sequence lifetime."
BB&T Bank building at the corner of Connecticut Avenue and I Street NW. Washington, D.C. 19 January 2013
© Luca Faccio - "Verhüllter Reichstag", or "Wrapped Parliament", an environmental artwork by Christo and Jeanne-Claude (Reichstag, Berlin, 1995)
The Reichstag lost its function as a democratic chamber in July 1933 and reacquired it on 7 September 1999
These vertical digital art transparencies were the original creations that i later turned into horizontals for wall decoration decals.
NAT-BALLOT-TRANSPARENCY
Saul Seyler, Ada County Elections Director in the warehouse of the Ada County Elections Office in Boise, Idaho November 20, 2024. Seyler is posing in an aisle with ballots from previous elections. Photo by Natalie Behring for the New York Times
Octobers theme was TRANSPARENCY and our speaker the awesome Peter Sunde. Happy to have you with us and sharing your story! Special thanks to our hosts Stpln - Stapelbädden and our global partners Wix, MailChimp and Shutterstock. Thanks for the fika, Love Coffee Roasters and Bethany Osment. #CMtransparency. All images by the brilliant Emilia Stålhammar.