RELEASE: H99-107

STARRY BULGES YIELD SECRETS TO GALAXY GROWTH

NASA's Hubble Space Telescope is uncovering important new clues to a galaxy's birth and growth by peering into its heart --a bulge of millions of stars that resemble a bulbous center yolk in the middle of a disk of egg white.

Hubble astronomers are trying to solve the mystery of which came first: the stellar disk or the central bulge?

Two complementary surveys by independent teams of astronomers using Hubble show that the hubs of some galaxies formed early in the Universe, while others formed more slowly, across a long stretch of time.

Hubble confirms that the evolutionary paths of bulges and disks are connected. The central bulge stabilizes a galaxy's development and largely controls the ebb and flow of star birth in the core. The central bulge holds secrets as to how and when a galaxy formed. Before Hubble, astronomers had detailed information only about the complex core of our galaxy, which has a small bulge peppered with massive young star clusters and a telltale bar structure funneling gas to the center. Hubble allows astronomers to see bright star clusters, bars and other structures deep inside the bulges of other galaxies.

A group led by Reynier Peletier from the University of Nottingham, in the United Kingdom, has confirmed that the central
bulges of more tightly wound spirals were all created at more or less the same time in the early universe.

A second team, led by C. Marcella Carollo of Columbia University in New York, surveyed galaxies that have small bulges
and bar-like structures that bisect the nucleus like the slash across a no-smoking sign. They found that the bulges in these
galaxies grew more recently, through markedly different processes happening within the galaxy's disk.

Both surveys used Hubble's precise resolution to peer into bulbous hubs of more than 200 neighboring galaxies, out to a
distance of 100 million light-years. Using Hubble's visible-light and infrared cameras to penetrate deep into the cores of the
galaxies, astronomers were able to untangle the stars' true colors -- a measure of age -- from their apparent colors, which are made redder by interstellar dust.

Peletier's team used Hubble to look into the center of 20 spiral galaxies that have large bulges. The team found that
elliptical bulges of stars formed over a relatively brief period very early in the young universe. This could have happened
through the collapse of a single cloud of hydrogen or merger of primeval star clusters.

"Apparently everywhere in the universe these intermediate-sized galaxies must have started forming early on," reports
Peletier in a paper to be published in the Monthly Notices of the Royal Astronomical Society. "The bulges of early spiral galaxies are old, and at least the outer parts of their disks are considerably younger."

Carollo's team found that in a different class of spiral galaxy, a small bulge probably formed early on, but was later fed
by gas flowing into the galaxy's core, likely along a bar-like structure caused by instabilities in the surrounding disk of
stars. The gas fueled the birth of new stars, and the bulge inflated like a beach ball as brilliant star clusters populated
the center.

Carollo's results, to be published in the Astrophysical Journal, show young and old stars in the bulge. The researchers
say that these types of bulges can continue to grow in galaxies in the present universe, but it is unlikely that they will ever
become as big as those giant bulges that formed when the universe was young.

The Space Telescope Science Institute is operated by the Association of Universities for Research in Astronomy, Inc. for
NASA, under contract with NASA's Goddard Space Flight Center, Greenbelt, MD. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency.


NOTE TO EDITORS: Image files are available on the Internet at:

http://oposite.stsci.edu/pubinfo/latest.html

http://oposite.stsci.edu/pubinfo/pr/1999/34/pr-photos.html