Do Black Holes Prevent Starbirth?

Not Always

If you know anything about black holes (and you probably have at least heard that these bad boys suck up pretty much anything that wanders past their event horizons), then it might surprise you to learn that young stars can form near black holes. Now, this seems counter-intuitive, since, if the black hole is gobbling all the stuff up (including the stuff that makes stars), there wouldn’t be any (or at least enough) left to make stars.

Not so fast, says a team of astronomers and astrophysicists at the University of St. Andrews and University of Edinburgh in Scotland, U.K. It turns out that, through a set of computer simulations (left) of giant clouds of gas being sucked into black holes, the scientists have solved the mystery of how stars could be formed in the blustery, dangerous, and not completely hospitable environment near a black hole

The discovery of hundreds of high-mass young stars orbiting the black hole at the center of our own Milky Way was probably one of the most exciting in recent times. But, it begged the question of how they could have formed near the hungry maw of the black hole. And survived!

The series of images at  left show the evolution of a 10,000 solar-mass molecular cloud falling toward a supermassive black hole. Although the cloud is disrupted by the black hole, some of the material is captured to form an eccentric disc that quickly forms numerous stars. The stars that form retain the eccentricity of the captured gas and those that form very close to be the black hole tend to be very massive. These results match the two primary properties of the young stars that have formed in the center of the Milky Way Galaxy. They have high mass and they follow eccentric orbits around the supermassive black hole. Not only does this simulation set help us understand the black hole at OUR galaxy’s heart (and the formation of stars nearby), but they should be quite valuable when astronomers look to the hearts of other galaxies and find newborn stars orbiting close to the hungry maws of supermassive black holes.

Hubble’s Magnetic Monster

The Power of Magnetic Fields in Space

Yesterday this amazing picture came rumbling through the Intarwebs from the folks at Hubble Space Telescope. It’s from the Advanced Camera for Surveys and shows the galaxy NGC 1275 seemingly surrounded by what looks like a spiderweb of stuff.

Now, there’s a lot going on here, so let’s break it down. First, the galaxy is in the center of the Perseus Cluster of galaxies, and the whole region is permeated with hot gas — REALLY hot — around 100 million degrees. The red stringy things are filaments of cooler hydrogen gas and they’re threaded on magnetic field lines that extend throughout the region.

Magnetic field lines?  Yes, this is indeed true. The actions of a supermassive black hole and its associated jet at the core of the galaxy are the source of very strong magnetic fields that extend quite far out from the core. Gas near the center of the galaxy gets superheated by all the hoopla surrounding the black hole and jet, and that blows bubbles of material out into surrounding space. Those expanding bubbles plow into cooler regions of hydrogen gas, and the expansion carries some of that gas out along with it. The red filaments are the hydrogen gas that looks like it’s draped on the magnetic field lines. Those filaments are actually a very important clue to astronomers. They are the biggest visible-light evidence for some “invisible” (i.e. not visible to our eyes) interactions between NGC 1275’s central black hole and the hot gas that permeates the surrounding interstellar and intergalactic spaces.

Now, the filaments look really delicate, and you’d think that the huffing and puffing of material blasting out from the center of the galaxy via the jet would destroy the hydrogen gas threads. What’s saving them are the magnetic fields. Those lines of force hold the gas in place and help it resist the outward blasts from the core of the galaxy. They also keep the gas from clumping up to form newborn stars, making them a disruptive as well as a unifying force.

For anybody who thought that intergalactic space might be empty and boring, this image and another one taken with multiple instruments (left), reveals just how frenetic the environment in galaxy clusters can be.

While we may not be able to see those magnetic fields, images like these show us the effects that such fields have on the ordinary matter they thread through.

For more information, surf on over to the Space Telescope Science Institute’s HubbleSite page.