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Stellar Astrophysics for the Local Group
A review of the new subject of extragalactic stellar astrophysics - for both graduate students and researchers working in astrophysics.
Wolf-Rayet Stars: Observations, Physics, Evolution
Proceedings of IAU Symposium No. 99, held at Cozumel, Mexico, September 18-22, 1981
Luminous Stars and Associations in Galaxies
Proceedings of the 116th Symposium of the International Astronomical Union, held at Porto Heli, Greece, May 26-31, 1985
Groups of Galaxies in the Nearby Universe
For every galaxy in the field or in clusters, there are about three galaxies in groups. The Milky Way itself resides in a group, and groups can be found at high redshift. The current generation of 10-m class telescopes and space facilities allows the observation of the members of nearby groups with exquisite detail, and their properties can be correlated with the global properties of their host group. Groups in the local Universe offer us the chance to study galaxies in environments characterized by strong interactions. In the cosmological context, groups trace large-scale structures better than clusters, and the evolution of groups and clusters appears to be related. All these aspects of research on groups of galaxies are summarized in this book written by scientists working in various fields.
Spiral Galaxies in the Near-IR
From June 7-9, 1995, the European Southern Observatory (ESO) and the Max Plank Institut fiir Astrophysik (MPA) jointly held the Workshop on Spiral Galaxies in the Near-IR. This meeting took place at the ESO headquarters in Garching bei Miinchen, Germany. The weather waschanging, with the biergarten closed, but that did not stop 85 people from allover the world from attending the meeting. The three days were intensive, with talks and coffee and posters from 9 am to 6 pm, and very productive indeed for everyone. The topics covered the stellar populations of the Milky Way and other more distant spirals, the role of dust, the dynamics of spiral galaxies, and the nuclear activity seen at near-IR ...
Nearly Normal Galaxies
It is sometimes said that astronomy is the crossroads of physics. In the same spirit, it can forcefully be argued that galaxies are the crossroads of astronomy. Internal pro ces ses within galaxies involve all of the fundamental components of astrophysics: stellar evolution, star formation, low-density astrophysics, dynamics, hydrodynamics, and high-energy astrophysics. Indeed, one can hardly name an observational datum in any wavelength range on any kind of celestial object that does not provide a useful clue to galaxy formation and evolution. Although internal processes in galaxies until recently occupied most of our attention, we now know that it is also vital to relate galaxies to their ...
Symposium
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Nuclei in the Cosmos III Third International Symposium on Nuclear Astrophysics
Annotation The July 1994 symposium was an international forum in which scientists working in different research branches connected to nucleosynthesis could discuss the most recent achievements in nuclear astrophysics. The topics addressed range from laboratory work of nuclear astrophysics, especially on reaction rates, to models of nucleosynthesis in single and double stars; from measurements of abundances and isotopic anomalies in pristine meteorites to the reconstruction of the early evolutionary phases of the Solar System; and from optical and radio spectroscopic studies of the composition in stellar atmospheres and circumstellar envelopes to modeling of the global chemical evolution of galaxies. No subject index. Annotation c. by Book News, Inc., Portland, Or.
