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Cited by 695

The DOI matches its Crossref record; 270 of the 270 references it cites were found in a registry or an index.

The ATLAS3D project – XX. Mass–size and mass–σ distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function

Open access
Cappellari, Michele, McDermid, Richard M., Alatalo, Katherine, Blitz, Leo, Bois, Maxime, Bournaud, Frédéric, Bureau, M., Crocker, Alison F., Davies, Roger L., Davis, Timothy A., de Zeeuw, P. T., Duc, Pierre-Alain, Emsellem, Eric, Khochfar, Sadegh, Krajnović, Davor, Kuntschner, Harald, Morganti, Raffaella, Naab, Thorsten, Oosterloo, Tom, Sarzi, Marc, Scott, Nicholas, Serra, Paolo, Weijmans, Anne-Marie, Young, Lisa M.·2013·Monthly Notices of the Royal Astronomical Society
DOI 10.1093/mnras/stt644
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Abstract

In the companion Paper XV of this series, we derive accurate total mass-to-light ratios (M/L) JAM ≈ (M/L)(r = R e ) within a sphere of radius r = R e centred on the galaxy, as well as stellar (M/L) stars (with the dark matter removed) for the volume-limited and nearly massselected (stellar mass M 6 × 10 9 M ) ATLAS 3D sample of 260 early-type galaxies (ETGs, ellipticals Es and lenticulars S0s).Here, we use those parameters to study the two orthogonal projections (M JAM , σ e ) and (M JAM , R maj e ) of the thin Mass Plane (MP) (M JAM , σ e , R maj e ) which describes the distribution of the galaxy population, where M JAM ≡ L × (M/L) JAM ≈ M .The distribution of galaxy properties on both projections of the MP is characterized by: (i) the same zone of exclusion (ZOE), which can be transformed from one projection to the other using the scalar virial equation.The ZOE is roughly described by two power laws, joined by a break at a characteristic mass M JAM ≈ 3 × 10 10 M , which corresponds to the minimum R e and maximum stellar density.This results in a break in the mean M JAM -σ e relation with trends M JAM ∝ σ 2.3 e and M JAM ∝ σ 4.7 e at small and large σ e , respectively; (ii) a characteristic mass M JAM ≈ 2 × 10 11 M which separates a population dominated by flat fast rotator with discs

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Metadata

Authors
Cappellari, M., McDermid, R. M., Alatalo, K., Blitz, L., Bois, M., Bournaud, F., Bureau, M., Crocker, A. F., Davies, R. L., Davis, T. A., de Zeeuw, P. T., Duc, P.-A., Emsellem, E., Khochfar, S., Krajnović, D., Kuntschner, H., Morganti, R., Naab, T., Oosterloo, T., Sarzi, M., Scott, N., Serra, P., Weijmans, A.-M., & Young, L. M.
Venue
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP)
Published
2013-05-16
Volume
432
Issue
3
Pages
1862-1893
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
DOI
10.1093/mnras/stt644
OpenAlex
W2086421432
Cited by
695
References
270
FWCI
36.28
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The ATLAS3D project – XX. Mass–size and mass–σ distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function. https://app.cochat.ai/papers/10.1093/mnras/stt644
The paper
Cappellari, M., McDermid, R. M., Alatalo, K., Blitz, L., Bois, M., Bournaud, F., Bureau, M., Crocker, A. F., Davies, R. L., Davis, T. A., de Zeeuw, P. T., Duc, P.-A., Emsellem, E., Khochfar, S., Krajnović, D., Kuntschner, H., Morganti, R., Naab, T., Oosterloo, T., . . . Young, L. M. (2013). The ATLAS3D project – XX. Mass–size and mass–σ distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/stt644

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