Steve Gottlieb
July 7th, 2013, 06:27 PM
PK 1-6.2 = PN G001.5-06.7 = ESO 457-2 = HD 167362
18 16 12.2 -30 52 08
V = 11.9 (central star in SIMBAD)
The "discovery" name of this nearly stellar planetary is from the 1940 paper by Pol Swings and Otto Struve: "HD 167363 , An object similar to Campbell's Hydrogen Envelope Star" available at at http://www.pnas.org/content/26/7/454.full.pdf
This young, very compact planetary contains a hydrogen-deficient central star displaying a carbon-rich emission-line spectra (WC) very similar to young, massive Wolf-Rayet stars. The central star is surrounded by a small dusty halo showing red [N II] lines. Campbell's Hydrogen Star, with a similar spectra, displays a striking red ring (in larger scopes).
Both Campbell's star and Swings-Struve 1 were actually discovered by Williamina Fleming at Harvard (ApJ, 2, 354) back in 1895! (she found Campbell's Star in 1890). As it was assumed this was a star and not a planetary, Dreyer did not assign it an IC number to either object.
Sw-St 1 was later rediscovered by Merrill at Mount Wilson in 1925, then by Pol Swings and Otto Struve at McDonald Observatory around 1940 and picked up once again at Mount Wilson in 1950 by Karl Henize. What a history! For more information see the 2001 paper "SwSt 1: an O-rich planetary nebula around a C-rich central star" at http://m.mnras.oxfordjournals.org/content/328/2/527.full
Jimi Lowrey mentioned this object to me a couple of nights ago at the Golden State Star Party in northeastern California as he happened to run across the 1940 Swings-Struve paper and wondered if it might display a reddish halo like Campbell's Hydrogen Star. We couldn't confirm a color, though the central star is certainly off-white (Paul Alsing thought it had a reddish tinge) and appears slightly "soft" at high power in my 24" f/3.7. Although situated in a rich Milky Way field, I was able to quickly identify it (without a finder chart) by "blinking" the field with an NPB filter.
The next day I checked my notes database and found I had first observed Sw-St 1 27 years ago (August 1986) with my 13" and commented "blinks very well with an H-Beta filter which dramatically dims all stars. Responds to an OIII filter but to a lesser extent."
Jimi and I, along with several others at the star party, reobserved Sw-St 1 again last night (SQM-reading of 21.6) and found the H-beta response startling -- stars were dimmed nearly 3 magnitudes, but Sw-St 1 shone steadily and dominated the rich field. Campbell's Hydrogen Star will also display this unusual response to an H-beta filter though not as dramatically.
Perhaps more southernly observers can confirm if this planetary displays a red halo, though as the halo is barely non-stellar, so this will probably be a very tough observation. Nevertheless, if you're looking to find another target to use your H-beta filter on besides the Horsehead and the California nebula, check out Swings-Struve 1!
"Give it a go and let us know!"
Good luck and great viewing!
18 16 12.2 -30 52 08
V = 11.9 (central star in SIMBAD)
The "discovery" name of this nearly stellar planetary is from the 1940 paper by Pol Swings and Otto Struve: "HD 167363 , An object similar to Campbell's Hydrogen Envelope Star" available at at http://www.pnas.org/content/26/7/454.full.pdf
This young, very compact planetary contains a hydrogen-deficient central star displaying a carbon-rich emission-line spectra (WC) very similar to young, massive Wolf-Rayet stars. The central star is surrounded by a small dusty halo showing red [N II] lines. Campbell's Hydrogen Star, with a similar spectra, displays a striking red ring (in larger scopes).
Both Campbell's star and Swings-Struve 1 were actually discovered by Williamina Fleming at Harvard (ApJ, 2, 354) back in 1895! (she found Campbell's Star in 1890). As it was assumed this was a star and not a planetary, Dreyer did not assign it an IC number to either object.
Sw-St 1 was later rediscovered by Merrill at Mount Wilson in 1925, then by Pol Swings and Otto Struve at McDonald Observatory around 1940 and picked up once again at Mount Wilson in 1950 by Karl Henize. What a history! For more information see the 2001 paper "SwSt 1: an O-rich planetary nebula around a C-rich central star" at http://m.mnras.oxfordjournals.org/content/328/2/527.full
Jimi Lowrey mentioned this object to me a couple of nights ago at the Golden State Star Party in northeastern California as he happened to run across the 1940 Swings-Struve paper and wondered if it might display a reddish halo like Campbell's Hydrogen Star. We couldn't confirm a color, though the central star is certainly off-white (Paul Alsing thought it had a reddish tinge) and appears slightly "soft" at high power in my 24" f/3.7. Although situated in a rich Milky Way field, I was able to quickly identify it (without a finder chart) by "blinking" the field with an NPB filter.
The next day I checked my notes database and found I had first observed Sw-St 1 27 years ago (August 1986) with my 13" and commented "blinks very well with an H-Beta filter which dramatically dims all stars. Responds to an OIII filter but to a lesser extent."
Jimi and I, along with several others at the star party, reobserved Sw-St 1 again last night (SQM-reading of 21.6) and found the H-beta response startling -- stars were dimmed nearly 3 magnitudes, but Sw-St 1 shone steadily and dominated the rich field. Campbell's Hydrogen Star will also display this unusual response to an H-beta filter though not as dramatically.
Perhaps more southernly observers can confirm if this planetary displays a red halo, though as the halo is barely non-stellar, so this will probably be a very tough observation. Nevertheless, if you're looking to find another target to use your H-beta filter on besides the Horsehead and the California nebula, check out Swings-Struve 1!
"Give it a go and let us know!"
Good luck and great viewing!