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Beta Doradus
The AAVSO DSLR Observing Manual
Fundamental Parameters of Wolf-Rayet Stars VI
ESO Annual Report 2004 ESO Annual Report 2004 Presented to the Council by the Director General Dr
Gas and Dust in the Magellanic Clouds
2013 Version
Index to JRASC Volumes 61-90 (PDF)
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS. II
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS
The VLT-FLAMES Tarantula Survey ⋆⋆⋆⋆⋆⋆
Florida State University Libraries
The Wolf-Rayet Stars in the Large Magellanic Cloud? a Comprehensive Analysis of the WN Class
Early-Type Variables in the Magellanic Clouds. I. Beta Cephei Stars in The
The Star-Forming Complex LMC-N79 As a Future Rival to 30 Doradus
A Massive Nebula Around the Luminous Blue Variable Star RMC
Download This Article in PDF Format
Submillimeter to Centimeter Excess Emission from the Magellanic Clouds I
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS
The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turn-Offs
Top View
Publications for Peter Tuthill 2020 2019 2018
The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide
Annual Report / Rapport Annuel / Jahresbericht 1998
Identifying Young Stellar Objects in Nine Large Magellanic Cloud Star-Forming Regions
Surveying Outside the Solar System
Introduction to the Bright Cepheids Charts
ESO ASTROPHYSICS SYMPOSIA European Southern Observatory ——————————————————— Series Editor: Bruno Leibundgut S
The VLT-FLAMES Tarantula Survey
Cepheid Variable Stars
Core Processing Handle Core Data Reduction and Astrometric Data, E.G
Gamma Rays As Probes of Cosmic-Ray Propagation and Interactions in Galaxies
A Misty Cloud on Our Doorstep
The Fourth Catalogue of Population I Wolf-Rayet Stars in the Large Magellanic Cloud?
S Doradus Variables in the Galaxy and the Magellanic Clouds? A
The R136 Star Cluster Hosts Several Stars Whose Individual Masses
Additions to Astronomy-OP 2017
Properties of Extragalactic Wolf-Rayet Stars
A Collection of Curricula for the STARLAB Deep Sky Objects Cylinder & Slide Set Transcript
Weighing Melnick 34: the Most Massive Binary System Known
9 X13.5 Doublelines.P65
EDITORIAL O QUE É a REA? É Bem Provável Que Voce