COASTing to a sharper image.Astronomers have now combined the light from three small optical telescopes to make the sharpest visible-light image to date of a stellar system. The picture shows several times as much detail as the Hubble Space Telescope Hubble Space Telescope (HST), the first large optical orbiting observatory. Built from 1978 to 1990 at a cost of $1.5 billion, the HST (named for astronomer E. P. Hubble) was expected to provide the clearest view yet obtained of the universe. can reveal and 50 times more than any single telescope on Earth could discern. The largest such telescope is the 10-meter W.M. Keck Telescope in Hawaii. To accomplish that feat, researchers borrowed a technique from radio astronomy, in which an array of dish-shaped detectors acts as one large radio telescope. By combining light from a trio of telescopes spaced 6 meters apart at the Lord's Bridge Observatory near Cambridge, England, the scientists formed the equivalent of a single optical telescope as large as the total distance between the individual instruments. Last September, John E. Baldwin Professor John Evan Baldwin has worked at the Cavendish Astrophysics Group (formerly Mullard Radio Astronomy Observatory) since 1954. He played a pivotal role in the development of interferometry in Radio Astronomy, and later astronomical optical interferometry and lucky imaging. of the University of Cambridge and his colleagues used the combination telescope, known as COAST (Cambridge Optical Aperture Synthesis Telescope COAST, the Cambridge Optical Aperture Synthesis Telescope, is a multi-element optical astronomical interferometer with baselines of up to 100 metres, which uses aperture synthesis to observe stars with angular resolution as high as one thousandth of one arcsecond (producing ), to examine Capella, a double star system 40 light-years away. The two stars lie closer to each other than Earth does to the sun, but COAST images clearly separate the stars, track their orbital motion, and even show which member of the duo has a slightly higher luminosity luminosity, in astronomy, the rate at which energy of all types is radiated by an object in all directions. A star's luminosity depends on its size and its temperature, varying as the square of the radius and the fourth power of the absolute surface temperature. . Baldwin and his collaborators detail their work in the Feb. 1 Astronomy and Astrophysics Astronomy and astrophysics may refer to:
Astronomy and Astrophysics (abbreviated as A&A . Because it uses small telescopes with limited light-collecting area, COAST can bring its optics to bear only on the brightest stars. Baldwin says his team will soon add a fourth telescope to the array and will ultimately space the instruments as far apart as 100 m, improving resolution further. Naked came the quasars . . . not! A year ago, astronomers suggested that some of the brilliant beacons of light known as quasars were born naked, without a galaxy to swaddle swad·dle tr.v. swad·dled, swad·dling, swad·dles 1. To wrap or bind in bandages; swathe. 2. To wrap (a baby) in swaddling clothes. 3. To restrain or restrict. n. them (SN: 1/28/95, p. 56). That notion defies conventional wisdom, since quasars are thought to reside in host galaxies that fuel these powerful energy sources. Yet Hubble Space Telescope images of 11 of 15 nearby quasars showed no evidence of host galaxies. Announcing these results last year, John N. Bahcall John Norris Bahcall (December 30 1934 – August 17 2005) was an American astrophysicist. He is best known for his contributions to the solar neutrino problem and the development of the Hubble Space Telescope, and for his leadership and development of the Institute for Advanced of the Institute for Advanced Study in Princeton, N.J., said, "This is a giant step backwards in our understanding of quasars." It now appears that quasars aren't naked after all. At about the same time Hubble was picturing nearby quasars in visible light, Kim K. McLeod, now at the Smithsonian Astrophysical Observatory The Smithsonian Astrophysical Observatory (SAO) is a "research institute" of the Smithsonian Institution headquartered in Cambridge, Massachusetts, where it is joined with the Harvard College Observatory (HCO) to form the Harvard-Smithsonian Center for Astrophysics (CfA). in Cambridge, Mass., and George H. Rieke of the University of Arizona (body, education) University of Arizona - The University was founded in 1885 as a Land Grant institution with a three-fold mission of teaching, research and public service. in Tucson, were examining many of the same quasars in the near infrared, using a telescope at the Steward Observatory near Tucson. The images reveal fuzzy blobs that fit the description of host galaxies. Moreover, when McLeod manipulated some of the Hubble images to distinguish more clearly between the quasars and their environs, she discerned some of the same fuzzy blobs. Follow-up observations at Steward revealed host galaxies in most images analyzed by Bahcall's team, McLeod and Rieke reported in the Dec. 1, 1995 Astrophysical Journal Letters. Why should near-infrared telescopes on the ground spot host galaxies any better than Hubble, which flies above Earth's blurring atmosphere? McLeod and Rieke note that in the infrared, galaxies tend to be brighter and quasars dimmer dim·mer n. 1. A rheostat or other device used to vary the intensity of an electric light. 2. a. A parking light on a motor vehicle. b. A low beam. , making it easier to pick out a galaxy. Moreover, Hubble's relatively small mirror can't readily detect objects of low surface brightness, including some of the host galaxies. Contrary to the widespread belief that certain types of quasars are always associated with certain types of galaxies, Bahcall's team presents Hubble images in the Feb. 1 Astrophysical Journal showing that a wide variety of galaxies plays host to different quasars. |
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