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Mapping new features of Milky Way's bulge.


Mapping new features of Milky Way's bulge

With their view already obscured by Earth's atmosphere “Air” redirects here. For other uses, see Air (disambiguation).

Earth's atmosphere is a layer of gases surrounding the planet Earth and retained by the Earth's gravity. It contains roughly (by molar content/volume) 78% nitrogen, 20.95% oxygen, 0.93% argon, 0.
, astronomers have a tough time peering through galactic dust for a penetrating look at the Milky Way's core. But in 1985, the Infrared Telescope infrared telescope

A telescope, similar in operation to an optical telescope, that is designed to detect infrared radiation. Because infrared radiation is emitted by warm objects, infrared telescopes need to be shielded from local heat sources, as by
 (IRT IRT Item Response Theory
IRT In Regard To
IRT Incident Response Team
IRT In Reference To
IRT In Regards To
IRT Icing Research Tunnel (wind tunnel)
IRT Interborough Rapid Transit
) headed past the atmospheric shroud and took its pictures from space. Flown on the shuttle, it returned with enough data to provide a detailed map of our galaxy's inner bulge.

While the IRT images are limited to one wavelength and equal the resolution of pictures so far obtained by the Cosmic Background Explorer Cosmic Background Explorer: see infrared astronomy.
Cosmic Background Explorer (COBE)

U.S. satellite that from 1989 to 1993 mapped the cosmic background radiation field. In 1964, microwave radiation was discovered that permeated the cosmos uniformly.
 (SN: 4/28/90, p.260), they capture a greater slice of the Milky Way Milky Way, the galaxy of which the sun and solar system are a part, seen as a broad band of light arching across the night sky from horizon to horizon; if not blocked by the horizon, it would be seen as a circle around the entire sky.  in the northern celestial hemisphere. An already established calibration between detected light signals and their intensity enabled Stephen M. Kent and his co-workers at the Harvard-Smithsonian Center for Astrophysics The Harvard-Smithsonian Center for Astrophysics (CfA) is located in Cambridge, Massachusetts. It consists of the Harvard College Observatory and the Smithsonian Astrophysical Observatory. The Center is located at 60 Garden Street.  in Cambridge, Mass., to compare IRT's Milky Way maps with images of similar spiral galaxies that appear face-on as viewed from Earth. Such comparisons, says Kent, "can help fill in the missing blanks" about galactic structures, hinting at the three-dimensional character of Milky Way features visible only edge-on when viewed from Earth's vicinity.

Kent and his colleagues find evidence that gas in the Milky Way's inner bulge -- about 3,300 light-years in diameter -- may move in an elliptical el·lip·tic   or el·lip·ti·cal
adj.
1. Of, relating to, or having the shape of an ellipse.

2. Containing or characterized by ellipsis.

3.
a.
 orbit, indicating the bulge is much less symmetric than previously thought. He notes that the bulges of other spiral galaxies, including the nearby M31, also show asymmetry. In addition, Kent says the work supports the notion that a star cluster exists just a few light-years from the galactic center. Several scientists have suggested that such a cluster, also seen near the center of other spiral galaxies, may be caused by a black hole lurking at the Milky Way's core.

The team also discovered clues to a Milky Way feature that has no obvious counterpart in other spiral galaxies: an apparent ring of stars about 13,000 light-years from the center. Kent believes this may be an edge-on view of one of the Milky Way's spiral arms.

He and his co-workers, who discussed their initial findings at a conference in Chile last year, are preparing an expanded report for publication.
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Copyright 1990, Gale Group. All rights reserved. Gale Group is a Thomson Corporation Company.

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Author:Cowen, Ron
Publication:Science News
Date:Jun 2, 1990
Words:364
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