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Spiral Galaxies Ron Buta University of Alabama
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What are spiral galaxies? l Flattened systems of stars, gas, and dust l stars seem to concentrate in spiral “arms” l all bound by gravity into a single unit l typical size:50,000-100,000 light years l typical mass: 10billion-500billion suns l often there is also a prominent bulge
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Face-on spiral galaxy
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Highly inclined spiral galaxy
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Edge-on spiral galaxy
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Edge-on Spiral Galaxy
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Why are spirals interesting? l An intriguing morphology l difficult to explain l common and widespread thoughout the Universe l new stars tend to form in spirals but not in other types of galaxies l part of process of galaxy evolution and interaction l our Galaxy is a spiral
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Discovery of Spirals l 1845 William Parsons, Third Earl of Rosse, Ireland l 72-inch reflector l visually detected spiral arms in the Whirlpool Nebula M51 l many other “nebulae” found to be spirals
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William Parsons, “Lord Rosse” 1800-1867
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Discovery of spiral structure in M51
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What causes spiral structure? l Natural phenomenon in flat, rotating stellar disks l possibly triggered by an interaction with another galaxy l or generated by bars l “density waves”
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Spiral galaxy research at UA l morphology l sense of winding of spiral arms l gravitational torques due to bars and spiral arms l star formation in galactic rings
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The de Vaucouleurs Atlas of Galaxies Gerard de Vaucouleurs 1918-1995
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The de Vaucouleurs Atlas: what is it? l Authors: R. J. Buta (U. Alabama) l H. G. Corwin, Jr. (Caltech) l S. C. Odewahn (U. Arizona) l publisher: Cambridge Univ. Press l Purpose: to illustrate the de Vaucouleurs revised Hubble classification system with modern digital images
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NGC 7457 SA(rs)0-
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NGC 1553 SA( r )0
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NGC 1291 (R)SB(s)0/a
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NGC 2713 (R’)SB(rs)ab
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NGC 4736 (R)SA( r )ab
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NGC 5850 SB( r )b
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NGC 4501 (M88) SA(rs)b
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NGC 4321 (M100) SAB(s)bc
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NGC 1566 SAB(s)bc
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NGC 6643 SA(rs)c
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NGC 7479 SB(s)c
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NGC 6946 SAB(rs)cd
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NGC 5585 SAB(s)d
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NGC 4618 SB(rs)m
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Sense of winding of spiral arms l Trailing arms: follow direction of rotation l Leading arms: oppose direction of rotation l most spiral arms trail l but one galaxy has leading arms!
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Trailing arm spiral M81
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Leading arm spiral galaxy NGC 4622
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Barred spiral galaxies l A bar-like pattern of old stars crosses the center l arms break from the ends of this bar l 70% of spirals have a bar, including the Milky Way
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Barred spiral galaxy NGC 1365
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Barred spiral NGC 1300
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How stars move in presence of a bar l In solar system, planets follow elliptical paths with Sun at one focus l no torque on planet as it orbits l in presence of a bar, star may follow a centered elliptical orbit l there is a torque on star as it orbits l amount of torque is a measure of “bar strength”
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Rings of Star Formation l Real bar orbit l “lit up” by new stars l often not circular
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Gallery of spirals from the Hubble Space Telescope
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Typical spiral galaxy: NGC 4414
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Starburst spiral galaxy NGC 3310
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Ringed spiral galaxy NGC 7742
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Superposed spiral galaxies NGC 3314
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Edge-on spiral galaxy ESO 510-13
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Edge-on spiral galaxy NGC 4013
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Peculiar ring galaxy: Hoag’s Object
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Barred spiral galaxy NGC 4319 with quasar
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Polar ring galaxy NGC 4650A
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Compact galaxy group
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Colliding spiral galaxies: NGC 6745
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The Spiral Menagerie: Visual Observations of Spirals from McDonald and Siding Spring Observatories l 1977-1984 l photoelectric galaxy photometry runs l McDonald 30, 36, 82, and 107-inch telescopes l Siding Spring 40-inch telescope
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NGC 5194-5 (M51) - McDonald 30-inch
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NGC 1566, SSO 40-inch
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NGC 2403, McD 30-inch
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NGC 3034 (M82), McD 36-inch
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NGC 3893(36McD), 4449(36McD), 4676(107McD), 3646(36McD), and 5921(36McD)
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NGC 4631 (left) and NGC 4565(right) (both 30McD)
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M99, M100, M88, and M61 (all 30McD)
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M77(36McD), NGC4535(30McD), NGC5394-5(36McD), NGC3395-6(36McD), NGC5426- 7(36McD), NGC5247(36McD)
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Thank you!
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