Cookie consent

AstroBin saves small pieces of text information (cookies) on your device in order to deliver better content and for statistical purposes. You can disable the usage of cookies by changing the settings of your browser. By browsing AstroBin without changing the browser settings, you grant us permission to store that information on your device.

I agree
Contains:  B144, Sh2-101
Getting plate-solving status, please wait...

Tulip Nebula in Narrow Band with Cygnus X-1 Bow Shock

Technical card


Dates:June 16, 2020June 17, 2020June 18, 2020

Frames:
Astrodon Tru-Balance 1.25" 5nm HA: 88x300" (gain: 139.00) -10C bin 1x1
Astrodon Tru-Balance 1.25" 5nm OIII: 79x300" (gain: 139.00) -10C bin 1x1
Astrodon Tru-Balance 1.25" 5nm SII: 86x300" (gain: 139.00) -10C bin 1x1

Integration: 21.1 hours

Avg. Moon age: 25.95 days

Avg. Moon phase: 14.30%


Astrometry.net job: 3647381

RA center: 19h 59' 52"

DEC center: +35° 21' 42"

Pixel scale: 0.862 arcsec/pixel

Orientation: -101.289 degrees

Field radius: 0.695 degrees


Resolution: 3520x4621

Locations: Backyard, Tucson, Arizona, United States

Data source: Backyard

Description

The Tulip Nebula designated as Sh2-101 is a hydrogen emission nebula located 6000 light years away in the constellation Cygnus the Swan. This region is also home to the first stellar mass black hole discovered, Cygnus X-1. You can't see Cygnus X-1, but you can see its effect on its dusty surroundings. The blue OIII arc, top center, is the bow shock produced by a relativistic jet emitted from Cygnus X-1 colliding with the interstellar medium (ISM).

The APOD in the following link provides a nice roll-over, graphical annotation of this configuration: https://apod.nasa.gov/apod/ap090608.html

The relativistic jet appears to be emanating from star hd226868, a blue super giant variable. But, this giant is the companion of Cygnus X-1 which orbits it at 0.2AU. Matter siphoned off from the star forms an accretion disc around the black hole. This material is heated to millions of degrees, some of which escapes in jets perpendicular to the accretion disc. The ISM is not as thick on the opposite side of the black hole, so you don't see a corresponding bow shock in my image.

I chose to image the Tulip in narrow band hoping detect the black hole bow shock. I used a custom narrow band mix from Steve Milne that I find fairly natural looking. The formula for the mix is:

R: 0.5Ha + 0.5SII
G: 0.15Ha + 0.85OIII
B: OIII

I took this data over several nights from 6/16/2020 to 6/23/2020. On the night of 6/12, my wife and I were watching a thunderstorm in the mountains behind our house in which there were several very close ground strikes. Those lighting strikes became the Bighorn fire in Tucson and have burned 107,000 acres so far. While the winds were out of the south, I was able to image. But when the winds shifted to the north the smoke blew into the Tucson Valley. So the above data was taken while dodging wild fire smoke. At one time we had packed up to be ready to flee the fires. Luckily we didn't have to evacuate. So far the forest service has done a great job managing the fire and no dwellings have been destroyed. If my version of the Tulip looks a bit fiery, now you know why ; )

I grew up reading Astronomy magazine with its speculation that Cygnus X-1 would be considered the first discovered black hole. This was a time when quasars were mystery objects and not know to be active galactic nuclei (AGN) powered by super massive black holes. Cygnus X-1 inspired a Rush song in two parts: Cygnus X-1 Book 1, The Voyage on "A Farewell to Kings" and Book 2, Hemispheres on the Hemispheres album of which I was a big fan. Cygnus X-1 represents the confluence of my teenage interests in astronomy, science fiction and music.

Comments

Author

andrewjbarton
Andrew Barton
License: Attribution Creative Commons
1503
Like

Sky plot

Sky plot

Histogram

Tulip Nebula in Narrow Band with Cygnus X-1 Bow Shock, 



    
        

            Andrew Barton