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NGC 1852

  • Expected Differences Between AGB Stars in the LMC and the SMC Due to Differences in Chemical Composition

    Expected Differences Between AGB Stars in the LMC and the SMC Due to Differences in Chemical Composition

  • Arxiv:1802.01597V1 [Astro-Ph.GA] 5 Feb 2018 Born 1991)

    Arxiv:1802.01597V1 [Astro-Ph.GA] 5 Feb 2018 Born 1991)

  • Ngc Catalogue Ngc Catalogue

    Ngc Catalogue Ngc Catalogue

  • Arxiv:1803.10763V1 [Astro-Ph.GA] 28 Mar 2018

    Arxiv:1803.10763V1 [Astro-Ph.GA] 28 Mar 2018

  • 19 91Apjs. . .76. .185E the Astrophysical Journal Supplement

    19 91Apjs. . .76. .185E the Astrophysical Journal Supplement

  • Chemical Evolution of the Large Magellanic Cloud)

    Chemical Evolution of the Large Magellanic Cloud)

  • Dust-Enshrouded Giants in Clusters in the Magellanic Clouds Stellar Dust Emission Are Essential to Measure the Mass-Loss Rate from These Stars

    Dust-Enshrouded Giants in Clusters in the Magellanic Clouds Stellar Dust Emission Are Essential to Measure the Mass-Loss Rate from These Stars

  • INFRARED SURFACE BRIGHTNESS FLUCTUATIONS of MAGELLANIC STAR CLUSTERS1 Rosa A

    INFRARED SURFACE BRIGHTNESS FLUCTUATIONS of MAGELLANIC STAR CLUSTERS1 Rosa A

  • Stars, Galaxies, and Beyond, 2012

    Stars, Galaxies, and Beyond, 2012

  • Statistical Analyses of Massive Stars and Stellar Populations

    Statistical Analyses of Massive Stars and Stellar Populations

  • Catalogue of Large Magellanic Cloud Star Clusters Observed in the Washington Photometric System

    Catalogue of Large Magellanic Cloud Star Clusters Observed in the Washington Photometric System

  • New Insights on the Bursting Formation of Star Clusters in the Large Magellanic Cloud � Andres´ E

    New Insights on the Bursting Formation of Star Clusters in the Large Magellanic Cloud Andres´ E

  • Universidade Federal Do Rio Grande Do Norte Centro De Ciências Exatas E

    Universidade Federal Do Rio Grande Do Norte Centro De Ciências Exatas E

  • Star Clusters with Dual Red Clumps 3 Quietly Burns Helium Thereafter

    Star Clusters with Dual Red Clumps 3 Quietly Burns Helium Thereafter

  • ESO Celebrates Its New Technology Telescope

    ESO Celebrates Its New Technology Telescope

  • Gamma Rays As Probes of Cosmic-Ray Propagation and Interactions in Galaxies

    Gamma Rays As Probes of Cosmic-Ray Propagation and Interactions in Galaxies

  • Durham Research Online

    Durham Research Online

  • A Revised and Extended Catalog of Magellanic System Clusters

    A Revised and Extended Catalog of Magellanic System Clusters

Top View
  • Fermi Large Area Telescope Fourth Source Catalog ABSTRACT We
  • Searching for Chemical Inhomogeneities in Open Clusters Analysis of the CN and CH Molecular Band Strengths in NGC 2158, NGC 2420, NGC 2682, NGC 7789, and Berkeley 29
  • Publisher Version (Open Access)
  • Astronomy and Astrophysics Library
  • Dust-Enshrouded Giants in Clusters in the Magellanic Clouds
  • Curriculum Vitae - Q
  • First Observational Signature of Rotational Deceleration in a Massive, Intermediate-Age Star Cluster in the Magellanic Clouds
  • IUE References from 1978 Until June 2001
  • Star Clusters with Dual Red Clumps
  • Blue Straggler Stars Beyond the Milky Way. III. Detection of Evolved Blue
  • Globular Clusters As Probes of Galaxy Formation
  • Advances in Understanding High-Mass X-Ray Binaries with INTEGRAL and Future Directions
  • Arxiv:1410.3840V3
  • X-Ray and Optical Observations of Globular Clusters and Pulsars
  • Multiple Stellar Populations in Magellanic Clouds Clusters


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