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NGC 2280
Strong Evidence for the Density-Wave Theory of Spiral Structure from a Multi-Wavelength Study of Disk Galaxies Hamed Pour-Imani University of Arkansas, Fayetteville
Atlas Menor Was Objects to Slowly Change Over Time
The Prairie Astronomer January, 2013 Volume 54, Issue #1 the Official Newsletter of the Prairie Astronomy Club
190 Index of Names
Making a Sky Atlas
Meeting Announcement Astro-Imaging Special Interest
Constraining Spiral Galaxy Mass Distributions with the Rss Imaging Spectroscopy Nearby Galaxy Survey
Cloud Download
The SPIRIT Telescopes
Dark and Luminous Matter in Bright Spiral Galaxies
Hind's Variable Nebula NGC1555 in Taurus
Logarithmic Spiral Arm Pitch Angle of Spiral Galaxies
A Abell 21, 20–21 Abell 37, 164 Abell 50, 264 Abell 262, 380 Abell 426, 402 Abell 779, 51 Abell 1367, 94 Abell 1656, 147–148
TABLE 4: Properties of Bars
Canis Major the Trusty Dog by Magda Streicher
[email protected]
Pos(SSC2015)009 Α , , D Greement Both with Pre- Velocity field of the Same I Persions
Revised Shapley Ames.Pdf
Cma – Objektauswahl NGC
Top View
The Carnegie-Irvine Galaxy Survey. I. Overview and Atlas of Optical Images
Some of the More Common Objects to View in PDF Format
7000 List by Name
Catalogue of One Thousand Galaxies