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A MINUET OF GALAXIES
This troupe of four galaxies, known
as Hickson Compact Group 87 (HCG 87), is performing
an intricate dance orchestrated by the mutual gravitational
forces acting between them. The dance is a slow,
graceful minuet, occurring over a time span of hundreds
of millions of years.
The Wide Field and Planetary Camera
2 on NASA's Hubble Space Telescope (HST) provides
a striking improvement in resolution over previous
ground-based imaging. In particular, this image
reveals complex details in the dust lanes of the
group's largest galaxy member (HCG 87a), which is
actually disk-shaped, but tilted so that we see
it nearly edge-on. Both 87a and its elliptically
shaped nearest neighbor (87b) have active galactic
nuclei which are believed to harbor black holes
that are consuming gas. A third group member, the
nearby spiral galaxy 87c, may be undergoing a burst
of active star formation. Gas flows within galaxies
can be intensified by the gravitational tidal forces
between interacting galaxies.
So interactions can provide fresh fuel for both
active nuclei and starburst phenomena. These three
galaxies are so close to each other that gravitational
forces disrupt their structure and alter their evolution.
From the analysis of its spectra,
the small spiral near the center of the group could
either be a fourth member or perhaps an unrelated
background object.
The HST image was made by combining
images taken in four different color filters in
order to create a three-color picture. Regions of
active star formation are blue (hot stars) and also
pinkish if hot hydrogen gas is present. The complex
dark bands across the large edge-on disk galaxy
are due to interstellar dust silhouetted against
the galaxy's background starlight. A faint tidal
bridge of stars can be seen between the edge-on
and elliptical galaxies.
HCG 87 was selected for Hubble imaging
by members of the public who visited the Hubble
Heritage website (http://heritage.stsci.edu)
during the month of May and registered their votes.
The HST exposures of the winning target were then
acquired in July 1999 by the Hubble Heritage Team
and guest astronomers Sally
Hunsberger (Lowell Observatory, Flagstaff, Arizona)
and Jane Charlton
(Pennsylvania State University).
Credit: NASA and The Hubble
Heritage Team (STScI/AURA)
Acknowledgment: S. Hunsberger (Lowell Obs.) and
Jane Charlton (Pennsylvania State U.) |