Atlas and catalogue of infrared sources in the Magellanic Clouds
Author(s)
Bibliographic Information
Atlas and catalogue of infrared sources in the Magellanic Clouds
Kluwer Academic Publishers, c1990
- : alk. paper
Available at 4 libraries
  Aomori
  Iwate
  Miyagi
  Akita
  Yamagata
  Fukushima
  Ibaraki
  Tochigi
  Gunma
  Saitama
  Chiba
  Tokyo
  Kanagawa
  Niigata
  Toyama
  Ishikawa
  Fukui
  Yamanashi
  Nagano
  Gifu
  Shizuoka
  Aichi
  Mie
  Shiga
  Kyoto
  Osaka
  Hyogo
  Nara
  Wakayama
  Tottori
  Shimane
  Okayama
  Hiroshima
  Yamaguchi
  Tokushima
  Kagawa
  Ehime
  Kochi
  Fukuoka
  Saga
  Nagasaki
  Kumamoto
  Oita
  Miyazaki
  Kagoshima
  Okinawa
  Korea
  China
  Thailand
  United Kingdom
  Germany
  Switzerland
  France
  Belgium
  Netherlands
  Sweden
  Norway
  United States of America
Note
Includes bibliographical references
Description and Table of Contents
Description
Around the beginning of the sixteenth century, Portuguese and Dutch sailors first ventured into southern seas. With their keen navigational interest in the skies, they noted the continuous presence of two cloud-like features, not far from the almost immediately Southern Pole. The first literature mention of these 'clouds' was in the journal written in 1520 by the Italian navigator Pigafetta on the first circumnavigation of the globe by Magalhaes (c/. Pigafetta et ai. , 1962). In honour of this exploit, the objects have since become known as the Magellanic Clouds, although the Dutch name 'Kaapsche Wolken' (Cape Clouds - after the Cape of Good Hope) has also been in use for centuries. The Large and Small Magellanic Clouds are dwarf irregular galaxies, orbiting our own Milky Way Galaxy, presently at distances of 53 and 63 kpc respectively (Humphreys, 1984) . . They are the galaxies nearest to us: most other Local Group galaxies are of order ten times more distant. The LMC and SMC are also the prototypical blue dwarf irregulars, representatives of a class of objects in which several hundred more distant objects are now known. Their masses are a few per cent of the mass of the Milky Way Galaxy, but they are relatively gas-rich and appear to be, at the present epoch, forming stars at a more prodiguous rate than our Galaxy (c/. Lequeux, 1984).
Table of Contents
1. Introduction.- 2. Infrared Source Identification Tables.- Table SMC-2.1: H? Nebulae.- SMC-2.2: Dark Clouds.- SMC-2.3: Stellar Objects.- LMC-2.1: H? Nebulae.- LMC-2.2: Dark Clouds.- LMC-2.3: Stellar Objects.- 3. The Leiden-IRAS Magellanic Clouds Infrared Source Catalogues.- Catalogue LI-SMC.- Catalogue LI-LMC.- 4. Atlas of Infrared Emission of the Magellanic Clouds.- Table SMC-4.1: Fields.- LMC-4.1: Fields.- SMC-4.2: Field Characteristics.- LMC-4.2: Field Characteristics.- SMC-4.3: Atlas Contour levels.- LMC-4.3: Atlas Contour levels.- Atlas SMC.- Atlas LMC.
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