The Formation of Galaxies First Presentation: The Hubble Sequence Bruno Berwanger Remco van der Burg Short Preview ► Edwin Hubble ► The Hooker Telescope ► What is the Hubble Sequence? ► Differences between known galaxy types ► Examples ► Summary Edwin Hubble (1889-1953) ► State Record high jump 1906 ► Served in both WWI and WWII ► 1919 A.D. Observations with Hooker Telescope ► 1953 Nobel prize The Hooker Telescope ► Built in 1908 ► Location: northeast of Los Angeles ► Mountain of 1742 meter high ► Resolving Power: 0.05” Tuning Fork Diagram Elliptical Galaxies (E0-E7) ► Degree of eccentricity ► Mostly consists of old stars ► Population II stars ► Low in gas and dust ► Physical Properties enormous range Examples NGC 4623 – E7 NGC 4365 – E3 Spiral Galaxies (Sa – Sd) ► Central bulge ► Outlying disk containing spiral arms ► Plenty of gas and dust ► Old and young stars ► Sa tightly wound + big central bulge ► Sd very loose spirals + small central bulge Spiral NGC 4448 - Sa NGC 5457 - Sc Barred Spiral Galaxies (SBa-SBd) ► Spirals running from a bar ► Plenty of gas and dust ► Old and young stars ► Bars temporary? Examples NGC 253 - SBc NGC 1300 - SBc Lenticular Galaxies (S0, SB0, E8) ► Intermediate between Elliptical and Spirals in: Composition Age of stars Shape NGC 4649 – E8 NGC 4684 – S0 Irregular Galaxies (Irr I, Irr II) ► Do not fit in the Hubble Classification ► Irr I Deformed Galaxies Sometimes remnants can be seen ► Irr II Completely Chaotic in form Mostly Young stars Will later take one of the regular shapes Examples Large Magellanic Cloud – Irr I Irr II Visible Galaxies ► All visible Galaxies: 77% Spirals 20% Elliptical 3% Irregular ► Within 9 Mpc from here: 33% Spirals 13% Elliptical 54% Irregular Some facts Ellipticals Spirals Irregulars m sun 105 to 1013 109 to 1011 108 to 1010 Abs Mag -9 to -23 -15 to -21 -13 to -18 Diameter (kpc) 1 to 200 5 to 50 1 to 10 Spectral Type K F to K A to F Summary ► The Hubble sequence is a usefull tool for the classification of galaxies: Elliptical Galaxies (Barred)Spiral Galaxies Lenticular Galaxies Irregular Galaxies The End
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