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User Guide

Published online by Cambridge University Press:  05 August 2015

Ronald Stoyan
Affiliation:
Interstellarum magazine
Stefan Binnewies
Affiliation:
Amateur astrophotographer
Susanne Friedrich
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Garching, Germany
Klaus-Peter Schroeder
Affiliation:
Universidad de Guanajuato, Mexico
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Summary

The data files

Degree of difficulty: rating of the observational difficulty:

  1. 1 object easily visible to the naked eye

  2. 2 object difficult to see with the naked eye

  3. 3 object easily visible in 8×30 binoculars

  4. 4 object easily visible in 10×50 binoculars

  5. 5 object difficult to see with 10×50 binoculars

For more information about visual and photographic difficulty, see page 63.

Minimum Aperture: minimum aperture required to see the object under a dark mountain sky, according to the personal experience of the first author. There are four categories:

  1. • naked eye

  2. • 15mm

  3. • 30mm

  4. • 50mm

Designation: catalog number in the NGC (New General Catalogue) or the IC (Index Catalogue).

Type: Object type. For a more detailed introduction to the different types, see page 53.

Class: Classification of the object, specific to its type:

  1. • Galactic nebulae: distinction between emission nebula and reflection nebula, see page 53

  2. • Open clusters: Trümpler classification, see page 55

  3. • Globular clusters: concentration class, see page 56

  4. • Galaxies: Hubble classification scheme, see page 61

Distance: Distance from Earth in light-years. As far as possible, uniform sources have been used, i.e.:

  1. • galactic nebulae and open clusters: K2005 (Kharchenko, N.V., et al.: “Astrophysical parameters of galactic open clusters,” Astronomy and Astrophysics 438, 1163 (2005)

  2. • globular clusters: R2005 (Recio-Blanco, A., et al.: “Distance of 72 galactic globular clusters,” Astronomy and Astrophysics 432, 851 (2005)

  3. • galaxies: H2000 (multiple authors: “The Hubble Space Telescope Key Project on the Extragalactic Distance Scale,” Astrophysical Journal 529, 698, 745, 786 (2000)

  4. • Virgo cluster galaxies: V2004 (Sanchis, T., et al.: “The origin of HI-deficiency in galaxies on the outskirts of the Virgo cluster. II. Companions and uncertainties in distances and deficiencies,” Astronomy and Astrophysics 418, 393 (2004)

  5. • Virgo cluster galaxies: V2002 (Solanes, J.M., et al.: “The Three-dimensional Structure of the Virgo Cluster Region from Tully-Fisher and HI data,” Astronomical Journal 124, 2440 (2002)

  6. • extragalactic HII regions: HK83 (Hodge, P.W., Kennicutt, R.C., Jr.: “An atlas of HII regions in 125 galaxies,” Astronomical Journal 88, pp.

Type
Chapter
Information
Atlas of the Messier Objects
Highlights of the Deep Sky
, pp. 10 - 14
Publisher: Cambridge University Press
Print publication year: 2008

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