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Family Traits of Galaxies: From the Tuning Fork to a Physical Classification in a Multi-Wavelength Context

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 435))

Abstract

At the time of the Great Debate nebulæ where recognized to have different morphologies and first classifications, sometimes only descriptive, have been attempted. A review of these early classification systems are well documented by the Allan Sandage’s review in 2005 (Sandage 2005 ). This review emphasized the debt, in term of continuity of forms of spiral galaxies, due by the Hubble’s classification scheme to the Reynold’s systems proposed in 1920 (Reynolds 1920 ).

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Notes

  1. 1.

    Editors Note: \(\lambda _{r}\) is a parameter describing the specific baryonic angular momentum defined as follows, \(\lambda _{r}\)=\(\langle r\vert V \vert \rangle /\langle r\sqrt{V ^{2 } +\sigma ^{2}}\rangle\), where r is the galacto-centric distance, V and \(\sigma\) are luminosity weighted averages of the rotation velocity and velocity dispersion over a two-dimensional kinematical field.

  2. 2.

    The “Sersic profile” is a photometric law empirically devised by Josè Luis Sersic in 1963 for fitting the luminosity profile of early-type galaxies:

    $$\displaystyle{I(r) = I_{0}\ exp(-(\frac{r} {\alpha } )^{ \frac{1} {n} })}$$

    where r is the radius, I the intensity, I 0 the intensity at the galaxy center, n the Sersic index, α the scale length.

  3. 3.

    Simple being here an advantage over the complex cameras generally used by professional astronomers that are subject to a larger number of instrumental artifacts.

  4. 4.

    [Note of the Editors] These observations used small size (0.16–0.58 m) private telescopes with large field of view (20.4×30.6–73.7×110.6 arcmin) with a scale in the range 0.4–1.66 arsec px−1.

  5. 5.

    http://astrocladistics.org/.

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Correspondence to Roberto Rampazzo .

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Rampazzo, R. et al. (2016). Family Traits of Galaxies: From the Tuning Fork to a Physical Classification in a Multi-Wavelength Context. In: D'Onofrio, M., Rampazzo, R., Zaggia, S. (eds) From the Realm of the Nebulae to Populations of Galaxies. Astrophysics and Space Science Library, vol 435. Springer, Cham. https://doi.org/10.1007/978-3-319-31006-0_3

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