By Terry D. Oswalt
ISBN-10: 9400756089
ISBN-13: 9789400756083
This can be quantity 6 of Planets, Stars and Stellar structures, a six-volume compendium of recent astronomical examine, masking topics of key curiosity to the most fields of up to date astronomy. This quantity on “Extragalactic Astronomy and Cosmology” edited via William C. Keel provides obtainable assessment chapters on Galaxy Morphology, Elliptical and Disk Galaxy constitution and sleek Scaling legislation, big name Formation in Galaxies, The Cool ISM in Galaxies, The effect of surroundings on Galaxy Evolution, Clusters of Galaxies, lively Galactic Nuclei, huge Scale constitution of the Universe, Distance Scale of the Universe, Galaxies within the Cosmological Context, Evolution of lively Galactic Nuclei, The Intergalactic Medium, and Cosmic Microwave historical past. All chapters of the instruction manual have been written by way of practising execs. They comprise enough historical past fabric and references to the present literature to permit readers to profit adequate a couple of distinctiveness inside astronomy, astrophysics and cosmology to start all alone functional examine initiatives. within the spirit of the sequence Stars and Stellar platforms released via Chicago college Press within the Nineteen Sixties and Nineteen Seventies, every one bankruptcy of Planets, Stars and Stellar structures can stand by itself as a primary evaluate of its respective sub-discipline, and every quantity can be utilized as a textbook or prompt reference paintings for complicated undergraduate or postgraduate classes. complex scholars astronomers of their roles as either teachers and researchers will welcome Planets, Stars and Stellar structures as a entire and pedagogical reference paintings on astronomy, astrophysics and cosmology.
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Additional info for Planets, Stars and Stellar Systems: Volume 6: Extragalactic Astronomy and Cosmology
Example text
NGC 1705, also shown in > Fig. 1-12, is similar but has a super star cluster near the center and obvious peculiar filaments. It is classified as a blue compact dwarf by Gil de Paz et al. (2003). Both galaxies are classified as amorphous by Sandage and Bedke (1994). IB(s)m IB(s)m IB(s)m IAB(s)m IAB(s)m Im Im Im I0 pec I0 pec ⊡ Fig. 1-12 Examples of irregular galaxies ranging in absolute blue magnitude from −14 to −18. The galaxies are (left to right): Row 1 – NGC 4449, 1569, 1156, DDO 50, and A2359-15 (WLM galaxy); Row 2 – IC 10, DDO 155, DDO 165, NGC 1705, NGC 5253.
NGC 5253 looks almost like a tilted S0 galaxy, yet it has no bulge at its center, nor any obvious lenses. Instead, the central area is an irregular zone of active star formation. The central zone was interpreted by van den Bergh (1980a) as “fossil evidence” for a burst of star formation, possibly triggered by an interaction with neighboring M83. This is a case where the de Vaucouleurs classification of I0 seems reasonable: NGC 5253 is an early-type galaxy with a central starburst, probably the youngest and closest example known (Vanzi and Sauvage 2004).
The galaxies are (left to right): Row 1 – NGC 4449, 1569, 1156, DDO 50, and A2359-15 (WLM galaxy); Row 2 – IC 10, DDO 155, DDO 165, NGC 1705, NGC 5253. The “pec” stands for peculiar. All images are B-band from the dVA Galaxy Morphology 1 6 Other Dimensions to Galaxy Morphology The de Vaucouleurs classification volume recognizes three principal aspects of galaxy morphology, but there are many more dimensions than three. Stage, family, and variety are the dimensions most clearly highlighted in blue-light images and have a wide scope.
Planets, Stars and Stellar Systems: Volume 6: Extragalactic Astronomy and Cosmology by Terry D. Oswalt
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