Large Magellanic Cloud

Superbubbles

In a galaxy teeming with spectacular objects, each so magnificent and cosmically grand, among the most spectacular are its superbubbles

Recycling on a cosmic scale

While the searing stellar winds of single massive stars can blow a small bubble, ranging in diameter from fractions of 1pc to a few pc, the combined stellar winds and subsequent supernovae explosions of the entire OB association’s massive members expand these bubbles into a superbubble, an enormous structure with a diameter of ~100 pc. (In a typical OB association roughly one supernova per million years occurs, and this rate will remain approximately constant over 50 million years – the lifetime of the lowest mass B stars likely to become supernovae). 

As the hot and compressed bubble of material expands it ploughs into the surrounding material compressing it as well and trigging new star formation at the edges of the superbubble. So while destructive forces shaped the superbubble, new stars are forming around the edges where the gas is being compressed. Like recycling on a cosmic scale, this next generation of stars will breathe fresh life into the supperbubble. Such is the power of superbubbles that if they are large enough they can blow through the entire galactic disk, releasing their energy into the surrounding galactic halo or even into the intergalactic medium.

The Cloud very generously provides us with sixteen of these exotic objects and from the sheer opulence of N11 to the phantom glow of N185… no two are alike except in their ability to enchant and fascinate. A couple of them (N11 and N44) are like looking at textbook examples of the stellar birth, life and death that forms a superbubble with their vast star-filled superbubble cavities carved out by the lives and deaths of an OB association’s most massive stars, and the next generation of stars being birthed in the dollops of bright H II regions around the edges where the gas is being compressed.

N44, full of shimmering and glittering light. Credit: NASA, ESA, V. Ksoll and D. Gouliermis (Universität Heidelberg), et al.

N70, a beautiful and ghostly superbubble. Credit and copyright: Dylan O’Donnell

N11 is packed to capacity with fascination. Credit: NASA; C. Aguilera, S. Points, and C. Smith (CTIO); and Z. Levay (STScI)

Observing superbubbles

In order to appreciate the astounding immensity, power, complexity and beauty of the superbubbles, one needs to first observe them at low magnification without a filter, for all, bar the extremely faint N185 and N186, are a truly beautiful sight with the glittering stars of the stellar associations powering them, and the beautiful and complex tapestry of nebulosity, glowing in varying intensity from a beautiful silky smokiness to startlingly bright.

And the radiance of these exquisite objects with a UHC filter is breath-taking – an elaborate mosaic of nebulae with every nuance of glowing nebulosity to explore – from impenetrable and brilliantly glowing knots with beautifully defined edges, to pools of swirling nebula infused with rich pearly shades and depth, to almost translucent patches whose undefined edges simply melt away into the background.

Once you have been captivated by their mystery and beauty and the sheer magnitude of what they are, these glorious superbubbles demand return trips. I find that subsequent visits are even better as a superbubble appears even more beautiful and fascinating than the memories of it burned into one’s mind. And there is always something more to see, even if it is but a strand of faint nebulosity one missed on a previous visit. Frankly, superbubbles ought to come with a warning… don’t go there, you won’t want to come back.

The location of the LMC’s superbubbles. This beautiful photo was taken by astronomer and astronaut Karl Henize in Bloemfontein, South Africa, in 1951

Scrollable Table

Location: LMC = Supergiant Shell. SP = Southern Periphery

Superbubbles

Name
Local OB Assoc.
RA
Dec
Size ly
Region
Location
N11
LH 9
04 56 51
-66 24 24
490x325
Northwest
Central Chart
N44
LH 47
05 22 07
-67 56 46
325x245
Northwest
Central Chart
N51A
LH 51, 54
05 28 06
-67 26 50
440x390
Northeast
Sextant LMC 4 S/P
N51D
LH 63
05 26 14
-67 30 18
210x160
Northeast
Sextant LMC 4 S/P
N57A
LH 76
05 32 24
-67 41 18
650x325
Northeast
LMC 4 S/P
N70
LH 114
05 36 11
-69 11 48
300x300
Northeast
Central Chart
N103
NGC 1850
05 08 54
-68 45 00
390x390
Bar
Chart 2
N105
LH 31
05 09 57
-68 53 31
290x95
Bar
Chart 2
N144
LH 58
05 26 45
-68 49 54
390x245
Northeast
LMC 3
N154
LH 81, 87
05 35 04
-69 43 25
590x390
Southeast
Central Chart
N158
LH 101, 104
05 39 33
-69 25 48
325x290
Southeast
LMC 2
N160
LH 103
05 39 46
-69 45 39
580x390
Southeast
LMC 2
N185
-
04 53 58
-70 00 53
300-365
Southwest
LMC 7
N186
-
04 59 45
-70 09 45
420x320
Southwest
LMC 8
N206
LH 66, 69
05 29 36
-71 00 00
350x350
Southwest
LMC 9
30 Doradus C
LH 90
05 36 11
-69 11 48
320x290
Southeast
30 Doradus

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