First cycle
degree courses
Second cycle
degree courses
Single cycle
degree courses
School of Science
ASTRONOMY
Course unit
ASTROPHYSICS 1
SC03100526, A.A. 2017/18

Information concerning the students who enrolled in A.Y. 2016/17

Information on the course unit
Degree course First cycle degree in
ASTRONOMY
SC1160, Degree course structure A.Y. 2008/09, A.Y. 2017/18
N0
bring this page
with you
Number of ECTS credits allocated 7.0
Type of assessment Mark
Course unit English denomination ASTROPHYSICS 1
Website of the academic structure http://astronomia.scienze.unipd.it/2017/laurea
Department of reference Department of Physics and Astronomy
Mandatory attendance
Language of instruction Italian
Branch PADOVA
Single Course unit The Course unit can be attended under the option Single Course unit attendance
Optional Course unit The Course unit can be chosen as Optional Course unit

Lecturers
Teacher in charge ENRICO MARIA CORSINI FIS/05

ECTS: details
Type Scientific-Disciplinary Sector Credits allocated
Core courses FIS/05 Astronomy and Astrophysics 7.0

Mode of delivery (when and how)
Period Second semester
Year 2nd Year
Teaching method frontal

Organisation of didactics
Type of hours Credits Hours of
teaching
Hours of
Individual study
Shifts
Lecture 7.0 56 119.0 No turn

Calendar
Start of activities 26/02/2018
End of activities 01/06/2018

Examination board
Examination board not defined

Syllabus
Prerequisites: Basic background in astronomy, physics, and scientific programming.
Target skills and knowledge: The course draws on the structure of both our own galaxy, the Milky Way, and external galaxies to tackle questions about their formation and evolution. The lectures emphasize the interplay between observations and theory in understanding the nature of the galaxies.
Examination methods: Written and oral examination.
Assessment criteria: The evaluation is based on the level of understanding of the concepts discussed in lectures and exercises and on the ability of using them to address problems concerning the phenomenology of galaxies.
Course unit contents: 1. STRUCTURE AND DYNAMICS OF THE MILKY WAY: Fundamental and Local Standard of Rest. Peculiar velocity, solar motion, solar apex. Proper stellar motions and radial speed in the solar environment. Velocity ellipsoid. Oort formula and rotation curve of the Milky Way. Bottlinger diagram. Hydrodynamic equations. Asymmetric drift. Stellar populations and spiral structure of the Milky Way.

2. MORPHOLOGY OF GALAXIES: Morphological classification of normal galaxies (Hubble, de Vaucouleurs, van den Bergh, Morgan). Morphological classification of peculiar galaxies (Arp, Vorontsov-Velyaminov). Morphology and luminosity. Morphology of the galaxies of the Local Group. Problems in morphological classification.

3. PHOTOMETRY OF GALAXIES: Surface brightness, integrated luminosity, curves of growth, isophotes, equivalent and effective radius, radial surface-brightness profiles. Isophotes shape, isophotal twisting, deviations from perfect ellipses, disky and boxy isophotes. Photometric profiles of elliptical galaxies and bulges of disk galaxies (Hubble, de Vaucouleurs, Oemler, Nuker, King, Sersic). Photometric profiles of disks (Freeman I and II), Freeman law, high and low surface-brightness galaxies. One-dimensional parametric photometric decompositions. Parametric photometric decompositions along more than one axis, bulge ellipticity, disk inclination. Two-dimensional parametric photometric decompositions. Some highlights of photometric decompositions (B/D ratio, nuclear disks). Photometric parameters of elliptical, S0, spiral, and irregular galaxies.

4. INTRINSIC SHAPE OF GALAXIES: Shape of elliptical galaxies, dust-lane ellipticals, equilibrium planes. Shape of disk galaxies, disk thickness. Apparent and intrisic flattening, inclination, distribution function of intrinsic flattenings.

5. KINEMATICS OF GALAXIES: Interstellar medium (ionized, neutral, molecular, and hot gas, dust). Gas kinematics. Redshift, rotation curve, systemic velocity, velocity dispersion. Deprojection of the observed velocity, rigid-body rotation, flat portion of the rotation curve. Stellar kinematics, line-of-sight velocity distribution, h3 and h4 coefficients. Nuclear disks of gas and dust, extended gas disks, kinematic decouplings.

6. MASS OF GALAXIES: Mass determination of spiral and elliptical galaxies using gas dynamics (ionized, molecular, neutral gas, X-ray halo). Mass determination of elliptical galaxies using stellar dynamics (Virial theorem, hydrodynamic equations). Mass-luminosity ratio, dark matter.

7. DISTANCE SCALE: Parallax, Baade-Wesselink method. Cepheids, RR Lyrae, Novae. Supernovae Ia, luminosity function of globular clusters and planetary nebulae. Tully-Fisher relation, Faber-Jackson relation, Dn-sigma relation. Distance of the Galactic center, LMC, M31, and Virgo cluster. Hubble law, Hubble constant.
Planned learning activities and teaching methods: Lectures and guided exercises on observational and theoretical topics related to the structure of galaxies. Some of the lectures and exercises are done at the Asiago Astrophysical Observatory.
Additional notes about suggested reading: All the slides and notes of the lectures are available in the course Moodle website.
Textbooks (and optional supplementary readings)
  • J. Binney, M. Merrifield, Galactic Astronomy. Princeton, NJ: Princeton University Press, 1998. Cerca nel catalogo
  • L. S. Sparke, J. S. Gallagher, Galaxies in the Universe. Cambridge: Cambridge University Press, 2000. Cerca nel catalogo
  • S. Phillips, The Structure and Evolution of Galaxies. Chichester: Wiley, 2005. Cerca nel catalogo
  • M. H. Jones, R. J. A. Lamboure, S. Serjeant (ed.), An Introduction to Galaxies and Cosmology. Cambridge: Cambridge University Press, 2015. Cerca nel catalogo