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61 Leonis

  • List of Easy Double Stars for Winter and Spring  = Easy  = Not Too Difficult  = Difficult but Possible

    List of Easy Double Stars for Winter and Spring  = Easy  = Not Too Difficult  = Difficult but Possible

  • The Evening Sky Map

    The Evening Sky Map

  • Lunar Mansion Names in South-West China

    Lunar Mansion Names in South-West China

  • Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem

    Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem

  • Reduced Maximum Mass-Loss Rate of OH/IR Stars Due to Overlooked Binary Interaction

    Reduced Maximum Mass-Loss Rate of OH/IR Stars Due to Overlooked Binary Interaction

  • Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem

    Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem

  • Starry Nights Typeset

    Starry Nights Typeset

  • Discovery of a Shell of Neutral Atomic Hydrogen Surrounding the Carbon Star IRC+10216

    Discovery of a Shell of Neutral Atomic Hydrogen Surrounding the Carbon Star IRC+10216

  • Extrasolar Planets and Their Host Stars

    Extrasolar Planets and Their Host Stars

  • Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem

    Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem

  • Lists and Charts of Autostar Named Stars

    Lists and Charts of Autostar Named Stars

  • Constellation Names and Abbreviations Abbrev

    Constellation Names and Abbreviations Abbrev

  • Constellations

    Constellations

  • Dissertation

    Dissertation

  • Mass Loss of Stars on the Asymptotic Giant Branch Mechanisms, Models and Measurements

    Mass Loss of Stars on the Asymptotic Giant Branch Mechanisms, Models and Measurements

  • A History of Astronomy, 139 Adhafera

    A History of Astronomy, 139 Adhafera

  • Arxiv:1902.09259V1 [Astro-Ph.SR] 25 Feb 2019 Hence Epitomizing Our Understanding of the Maximum Mass-Loss Rate Achieved During the Asymptotic Giant Branch (AGB) Phase

    Arxiv:1902.09259V1 [Astro-Ph.SR] 25 Feb 2019 Hence Epitomizing Our Understanding of the Maximum Mass-Loss Rate Achieved During the Asymptotic Giant Branch (AGB) Phase

  • A Comparison of the Twenty-Eight Lunar Mansions Between Dabaism and Dongbaism

    A Comparison of the Twenty-Eight Lunar Mansions Between Dabaism and Dongbaism

Top View
  • Appendix: for Beginners Only
  • Are Dust Shell Models Well-Suited to Explain Interferometric Data of Late-Type Stars in the Near-Infrared?
  • The Constellations and Asterisms of Petrus Apianus (1524–1536)
  • Prime Focus Newsletter Mitchell, Lunar Module Pilot on Apollo 14, Passed Away at and for Maintenance of the Website
  • Teleskop Be- Stens Geeignet
  • The Sidereal Times the Offi Cial Newsletter of the Albuquerque
  • Conception D'un Modèle De Visibilité D'étoile À L'oeil Nu. Application À L'identification Des Décans Égyptiens
  • Early Star Catalogues of the Southern Sky De Houtman, Kepler (Second and Third Classes), and Halley
  • Stories of the Stars: the History and Folklore of Tibetan Ethnoastronomy
  • Agbs, Post-Agbs and the Shaping of Planetary Nebulae


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