Some Notes on NGC 3603
Author | : D. Sher |
Publisher | : |
Total Pages | : 33 |
Release | : 1964 |
Genre | : Stars |
ISBN | : |
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Author | : D. Sher |
Publisher | : |
Total Pages | : 33 |
Release | : 1964 |
Genre | : Stars |
ISBN | : |
Author | : Mount Stromlo Observatory |
Publisher | : |
Total Pages | : 362 |
Release | : 1964 |
Genre | : Astronomy |
ISBN | : |
Author | : Australia. Parliament |
Publisher | : |
Total Pages | : 980 |
Release | : 1964 |
Genre | : Australia |
ISBN | : |
All printed Parliamentary papers common to both Houses are included in v. 2, etc.
Author | : Astronomical Society of Southern Africa |
Publisher | : |
Total Pages | : 432 |
Release | : 1999 |
Genre | : Astronomy |
ISBN | : |
Author | : Australian National University |
Publisher | : |
Total Pages | : 436 |
Release | : 1964 |
Genre | : |
ISBN | : |
Author | : Australia. Parliament |
Publisher | : |
Total Pages | : 992 |
Release | : 1964 |
Genre | : |
ISBN | : |
Author | : |
Publisher | : |
Total Pages | : 568 |
Release | : 2001 |
Genre | : Astronomy |
ISBN | : |
Author | : F. Palla |
Publisher | : Springer Science & Business Media |
Total Pages | : 242 |
Release | : 2006-07-06 |
Genre | : Science |
ISBN | : 3540316337 |
The book begins with a historical introduction, "Star Formation: The Early History", that presents new material of interest for students and historians of science. This is followed by two long articles on "Pre-Main-Sequence Evolution of Stars and Young Clusters" and "Observations of Young Stellar Objects". These articles on the fascinating problem of star formation from interstellar matter give a thorough overview of present-day theories and observations. The articles contain material so far unpublished in the astronomical literature. The book addresses graduate students and can be used as a textbook for advanced courses in stellar astrophysics.
Author | : C. de Loore |
Publisher | : Springer Science & Business Media |
Total Pages | : 581 |
Release | : 2012-12-06 |
Genre | : Science |
ISBN | : 940097910X |
The formative ideas for this symposium originated in 1978 at the IAU Symposium No. 83 on "Mass Loss and Evolution of O-type Stars" held at Qualicum Beach, Vancouver Island, Canada - WR stars generally figure prominently in O-star meetings and vice versa! Following general appro val by the IAU Executive Committee the initial ideas were cemented at a subsequent meeting, IAU Colloquium No. 59 on "The Effects of Mass Loss on Stellar Evolution", held at Miramare, Trieste, Italy in 1980, which was attended by the ma,jority of the present Scientific Organising Committee and at which meeting the outline programme for this symposium was formulated. 1981 was considered an appropriate year in which to hold a meeting on WR stars, since the last IAU Symposium devoted to this stellar class had been held a decade earlier, in Buenos Aires (IAU Sym posium No. 49), and during this intervening period a wealth of new observational material had been obtained for WR stars together with significant advances on the theoretical front. The venue for this sym posium was chosen from the requirement, which can be inferred from the above, that a meeting on 'hot' stars take place in an appropriate, sunny climate and followed upon the excellent suggestion of Dr. C. Firmani to hold the symposium in Mexico.
Author | : Marc Sauvage |
Publisher | : Springer Science & Business Media |
Total Pages | : 563 |
Release | : 2013-06-29 |
Genre | : Science |
ISBN | : 9401733112 |
Galaxies have a history. This has become clear from recent sky surveys which have shown that distant galaxies, formed early in the life of the Universe, differ from the nearby ones. New observational windows at ultraviolet, infrared and millimetric wavelengths (provided by ROSAT, IRAM, IUE, IRAS, ISO) have revealed that galaxies contain a wealth of components: very hot gas, atomic hydrogen, molecules, dust, dark matter ... A significant advance is expected due to new instruments (VLT, FIRST, XMM) which will allow one to explore the most distant Universe. Three Euroconferences have been planned to punctuate this new epoch in galactic research, bringing together specialists in various fields of Astronomy.