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Zeta Puppis
La Photosynthèse Serait Apparue Chez Certains Organismes Primitifs Entre 2.800 Et -2.400 Millions D’Années Si L’On En Croit Certaines Archives Géologiques Terrestres
Spectral Classification of Stars
A Mass-Loss Rate Determination for Zeta Puppis from the Quantitative Analysis of X-Ray Emission-Line Profiles
Star Formation in Bok Globules Ba Reipurth, Copenhagen University Observatory
Mass Loss from Hot Massive Stars
UV Spectroscopy of Massive Stars
Scientificastronomerdocumentati
1455189355674.Pdf
Three Proposed B-Associations in the Vicinity of Zeta Puppis
Proceedings of the 18Th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
Brightest Stars : Discovering the Universe Through the Sky's Most Brilliant Stars / Fred Schaaf
Chandra Detection of Doppler-Shifted X-Ray Line Profiles Rf Om the Wind of Zeta Puppis (O4f)
GUM NEBULA AS the FOSSIL STROMGREN SPHERE of the VELA X SUPERNOVA John C
The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide
Massive Stellar Winds Are Made of Tiny Pieces 5 February 2013
Blue Supergiant Star
A Detailed X-Ray Investigation of Ζ Puppis IV
Program Schedule and Abstract Book
Top View
Chandra Observations of Zeta
Massive Stars in the Galactic Context
Arxiv:0904.3078V2
The Life and Death of Stars
March 2018 BRAS Newsletter
Astrophysics1 [138 Marks]
UNIT 6: (Double Award) PHYSICS 2 HIGHER TIER SAMPLE
Annie Jump Cannon 07
Newsletter 116 of Working Group on Massive Star
Wenzelspr09.Pdf (3.509Mb)
Planetary Data
SL Paper 3 Markscheme
Announcements
Radio and Submillimetre Observations of Wind Structure in Ζ Pup Smooth and Spherically Symmetric Models Give for the Mass Table 1