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An Introduction to Dwarf Galaxies

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An Introduction to Dwarf Galaxies An introduction to dwarf galaxies Jörg Dabringhausen Univerzita Karlova Praha An introduction to dwarf galaxies Topics to be covered in this lecture: ● What is a (dwarf) galaxy, as opposed to a star cluster? ● What types of dwarf galaxies do exist (dwarf elliptical, dwarf spheroidal, ultra faint dwarf, ultra compact dwarf, dwarf irregular, etc.), what are the differences, and how are they related to each other (if at all)? ● What is the origin of dwarf galaxies (formation scenarios, primordial vs. secondary galaxies)? ● What are the stellar populations of (dwarf) galaxies (simple vs. composite, initial mass function)? ● What is the mass of galaxies, how is it estimated, and what can be learned from these estimates? What is a Galaxy? (any ideas…?) What is a Galaxy? NGC 6814 Is this a galaxy? ...of course it is! ...but why? ● mass? ● extension? ● Substructure? (spiral arms /star clusters) Image Credit: ESA/Hubble & NASA; Judy Schmidt What is a Galaxy? NGC 1399 What about this? ...this as well! ...similarities of large elliptical galaxies with spiral galaxies: ● in mass ● in extension ● They have substructure! (globular clusters) Image credit: Hubble Legacy Archive What is a Galaxy? What about this? Sculptor ...this is also an (elliptical?) galaxy! ...but much less massive and extended than NGC 1399. Image credit: ESO What is a Galaxy? NGC 4755 (“Jewel Box”) What about this? ...this is a star cluster! ...but why? ● smaller still than typical galaxies ● part of a galaxy ● Stars are the highest level of substructure Image credit: ESO What is a Galaxy? What about this? NGC 104 (47 Tucanae) ...this is considered a star cluster, too! ...but why? It has as many stars as a small galaxy, but also many properties typical for star clusters (...compact, no substructure other than stars, part of something that is Image credit: ESO definitely a galaxy) Galaxy or star cluster? The term “galaxy” was introduced about 100 years ago to describe stellar systems similar to the Milky Way in luminosity and extension. Later on, the known populations of galaxies and star clusters became ever more diverse, and the distinction therefore becomes more difficult: ● There are systems classified as galaxies even though they have less stars (and perhaps even mass) than a massive star cluster. 47 Tucanae – a very bright globular cluster Sculptor – a dwarf spheroidal ESO galaxy ESO Galaxy or star cluster? The term “galaxy” was introduced about 100 years ago to describe stellar systems similar to the Milky Way in luminosity and extension. Later on, the known populations of galaxies and star clusters became ever more diverse, and the distinction therefore becomes more difficult: ● Most galaxies have substructures (other than stars) but some don’t - but very young star clusters have such substructure, too! NGC 346 – a very young and bright star cluster Sculptor – a dwarf spheroidal Eso galaxy NASA, ESA and A. Nota Galaxy or star cluster? The term “galaxy” was introduced about 100 years ago to describe stellar systems similar to the Milky Way in luminosity and extension. Later on, the known populations of galaxies and star clusters became ever more diverse, and the distinction therefore becomes more difficult: ● Galaxies have complex stellar populations (different metal abundances and ages), but globular clusters do, too! Stellar isochrones – same metallicity, y y t i t i s different ages s o o n i n i m m u l u Stellar isochrones – l same ages, different VandenBerg+ (2014) Bertelli+ (2008) metallicities surface temperature surface temperature Galaxy or star cluster? The term “galaxy” was introduced about 100 years ago to describe stellar systems similar to the Milky Way in luminosity and extension. Later on, the known populations of galaxies and star clusters became ever more diverse, and the distinction therefore becomes more difficult: ● Galaxies have complex stellar populations, but globular clusters do, too! Color-magnitude diagrams of globular clusters (Milone+ 2010) Galaxy or star cluster? The term “galaxy” was introduced about 100 years ago to describe stellar systems similar to the Milky Way in luminosity and extension. Later on, the known populations of galaxies and star clusters became ever more diverse, and the distinction therefore becomes more difficult: ● Galaxies have complex stellar populations (different metal abundances and ages), but globular clusters do, too! Star formation histories of various dwarf galaxies around the Milky Way (Weisz+ 2014) – Their stellar populations did not form instantly! Galaxy or star cluster? The term “galaxy” was introduced about 100 years ago to describe stellar systems similar to the Milky Way in luminosity and extension. Later on, the known populations of galaxies and star clusters became ever more diverse, and the distinction therefore becomes more difficult: ● Star clusters are (almost) always bound NASA, ESA and to a galaxy, but A. Nota so are many dwarf galaxies – and thus substructure of a larger galaxy ESO ESA/Hubble & NASA; Judy Schmidt Galaxy or star cluster? The term “galaxy” was introduced about 100 years ago to describe stellar systems similar to the Milky Way in luminosity and extension. Later on, the known populations of galaxies and star clusters became ever more diverse, and the distinction therefore becomes more difficult: ● Star clusters are (almost) always bound to a galaxy, but so are many dwarf galaxies – and thus substructure of a larger galaxy Globular clusters are distributed around galaxies and usually bound to them, even though not directly Harris (1999) Harris (1999) within the actual galaxy Galaxy or star cluster? The term “galaxy” was introduced about 100 years ago to describe stellar systems similar to the Milky Way in luminosity and extension. Later on, the known populations of galaxies and star clusters became ever more diverse, and the distinction therefore becomes more difficult: Most dwarf ● Star clusters Weisz+ (2014) are (almost) galaxies in always bound the Local Group are to a galaxy, but so are many bound to one dwarf galaxies of its maJor – and thus galaxies – substructure of thus they are substructure! a larger galaxy Searching a criterion to distinguish galaxies from star clusters Stellar populations, extensions, presence of substructure, etc, by themselves are not sufficient to distinguish star clusters from galaxies – thus other criteria are needed … but which ones? A hint: Image credit: ESO 47 Tucanae – compare the a globular star cluster extensions of star clusters and galaxies with similarly sized stellar populations – many of the current suggestions for defining a galaxy are in fact The Small Magellanic Cloud – a dwarf galaxy related to that. Searching a criterion to distinguish galaxies from star clusters Searching a criterion to distinguish galaxies from star clusters NGC 1399 – large galaxy Hubble Sculptor – dwarf galaxy ESO 47 Tuc – star cluster ESO Searching a criterion to distinguish galaxies from star clusters The “Gilmore gap” (or valley): Most stellar systems have combinations of characteristic radii and stellar masses that set them either clearly lley re va below the Gilmore ilmo G valley (star clusters) or above it (galaxies) (Gilmore+ 2007) Searching a criterion to distinguish galaxies from star clusters The “Gilmore gap” (or valley): Most stellar systems have combinations of characteristic radii and stellar masses that set them either clearly lley re va below the Gilmore ilmo G valley (star clusters) or above it (galaxies) (Gilmore+ 2007) Criterion somewhat ambiguous for some obJects Note that some authors claim that the Gilmore valley is well populated with obJects The relaxation time is the time after which encounters between stars can have changed their initial velocities Searchinggalaxies a criterion from star to distinguishclusters(absolute value and direction) by order of itself. Galaxies can be considered as stellar systems where this y lle cannot have a v happened within the re o age of the Universe. ilm relaxation time G = Hubble time Galaxies can be considered as stellar systems where this cannot have happened within the age of the Universe. Searchinggalaxies a criterion from star to distinguishclustersThis implies however that galaxies would become star clusters as the universe ages. Criterion Also, the subdivision somewhat of the compact ambiguous for many objects systems seems somewhat artificial. relaxation time = Hubble time There is evidence for dark matter or non- standard gravity in stellar systems above the black line, but not for those below the line – this Searchinggalaxies a criterion from star to distinguishclustersprovides another criterion to distinguish galaxies from star clusters. Note however: The evidence for dark matter Definitely is based on stellar y lle no dark matter populations and internal a v below this line dynamics that are re o ilm relaxation time perhaps not fulfilled. G = Hubble time And the winner is: The “Gilmore gap”. At least for me, because: ● The relaxation time seems to subdivide the Searchinggalaxies a criterion from star to distinguishclusterscompact obJects artificially, and provides a time-dependent criterion ● The presence for dark matter / non-standard gravity in all obJects y above the black line is a lle a v matter of debate and by re o no means certain. ilm relaxation time G = Hubble time no dark matter And the winner is: The “Gilmore gap”. (at least for me.) ● The “Gilmore gap” is a observationally uncovered natural Searchinggalaxies a criterion from star to distinguishclustersfeature that separates star star clusters. There is however currently no common agreement on one of y these criterions. lle a v re o ilm relaxation time G = Hubble time no dark matter Note that the criteria imply each other to some extent. The large extensions that place galaxies above the Gilmore gap also imply: large relaxation times Searchinggalaxies a criterion from star to distinguishclusters● ● galaxies cover large volumes and thereby have the potential to contain much dark matter Low Internal y ● lle a accelerations, so that v re non-standard gravity may o ilm relaxation time set in.
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