Astronomers revise galaxy-formation
models with the discovery that early galaxies
could have grown fat - fast.
Slurping up cold streams of
star fuel, some of the Universe's first galaxies
got fat quickly, new observations suggest. The
findings could overturn existing models for
the formation and evolution of galaxies that
predict their slow and steady growth through
mergers.
Researchers using the Subaru
telescope in Hawaii have identified five distant
galaxy clusters that formed five billion years
after the Big Bang. They calculated the mass
of the biggest galaxy in each of the clusters
and found, to their surprise, that the ancient
galaxies were roughly as big as the biggest
galaxies in equivalent clusters in today's Universe.
The ancient galaxies should
have been much smaller, at only a fifth of today's
mass, based on galaxy-formation models that
predict slow, protracted growth. "That
was the reason for the surprise - that it disagrees
so radically with what the predictions told
us we should be seeing," says Chris Collins
of Liverpool John Moores University in Birkenhead,
UK. Collins and his colleagues publish the work
today in Nature1.
The work suggests that an earlier
modelling result may have correctly posited
a mechanism - a cold stream of star-nourishing
hydrogen gas - by which these first massive
galaxies grew so rapaciously2. Taken together,
the two results suggest that early galaxies
grew quickly through injections of gas, rather
than slowly through mergers. "We have a
whole different story now about how galaxies
form," says Avishai Dekel of the Hebrew
University in Israel and first author of the
earlier paper.
Hierarchy
undermined
For years, astronomers have
relied on a hierarchical model of galaxy formation.
It explained how small chunks of stars were
born in dense regions where cold dark matter
clustered. These galactic building blocks, through
mergers, would stack up and form the large massive
galaxies that are seen today. In recent years,
astronomers have tried to refine the models
by adding in the actual gas mechanics of star
formation.
But adding the gas mechanics
slowed down the rate of galaxy growth seen in
the models. That's because, as gas cools and
falls in to the star-birthing centre of a galaxy,
it's heated up. Shock waves are produced that
expand outwards to agitate and heat up new gas
on the periphery, preventing it from collapsing
and falling in to form new stars. "It's
a mechanism that quenches or stops star formation,"
says Dekel. So the models predicted that, to
reach the massive galaxy sizes seen today, galaxies
would have to steal their stars through mergers
- a slow process - rather than growing their
own.
But Dekel's models suggested
a way to turbocharge the early galaxies. They
found that veins of cold gas, clinging to filaments
of dark matter, could pierce the hot gas shell
of a growing galaxy and fuel its continued growth.
That would allow galaxies to reach massive proportions
quickly. So some astronomers are seeing the
new observations as evidence of the existence
of these cold gas streams. "This is another
important piece in the puzzle of how big galaxies
are assembled," says Avi Loeb, of the Harvard-Smithsonian
Center for Astrophysics in Cambridge, Massachusetts,
who was not affiliated with either study.
Adapt
or die?
It's not yet certain how much
of a readjustment the hierarchical model will
need if the observations hold up. Dekel says
that the basic model, describing the way dark
matter clumps and merges, is fine; only the
gas mechanics need to be adjusted for his cold
streams. But Collins says the underlying models
of dark-matter mergers could have problems.
"I think the problem could be more general
than just needing a tweaking."
But both agree that more work
needs to be done, and an obvious next step is
to search for filaments of cold gas streaming
into early galaxies. And Loeb says they may
already have been spotted. Since 2000, astronomers
have wondered about the origin of strange, glowing
blobs of hydrogen gas in distant, ancient corners
of the Universe. Loeb says that they share many
characteristics with the putative cold-gas streams3.
Now that the idea is catching on, many astronomers
are requesting time on bigger telescopes that
can make finer pictures of these 10-billion-year-old
objects. Loeb thinks the blobs will resolve
into filaments.
And then, he says, astronomers
will have a new tool to gauge the growth of
a galaxy. They'll also get to see the very first
ones while they are still in their nurseries.
"This could give you a direct image of
how a galaxy is being made."
NASA/JPL-Caltech
http://www.nature.com/news/2009/090401/full/news.2009.225.html