On the mass-to-light ratio of the local Galactic disc and the optical luminosity of the Galaxy

We measure the volume luminosity density and surface luminosity density generated by the Galactic disc, using accurate data on the local luminosity function and the vertical structure of the disc. From the well-measured volume mass density and surface mass density, we derive local volume and surface...

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Published in:Monthly notices of the Royal Astronomical Society Vol. 372; no. 3; pp. 1149 - 1160
Main Authors: Flynn, Chris, Holmberg, Johan, Portinari, Laura, Fuchs, Burkhard, Jahreiß, Hartmut
Format: Journal Article
Language:English
Published: Oxford, UK Blackwell Publishing Ltd 01-11-2006
Blackwell Science
Oxford University Press
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Abstract We measure the volume luminosity density and surface luminosity density generated by the Galactic disc, using accurate data on the local luminosity function and the vertical structure of the disc. From the well-measured volume mass density and surface mass density, we derive local volume and surface mass-to-light ratios (M/L) for the Galactic disc, in the bands B, V and I. We obtain M/L for the local column of stellar matter of (M/L)B= 1.4 ± 0.2, (M/L)V= 1.5 ± 0.2 and (M/L)I= 1.2 ± 0.2. The dominant contributors to the surface luminosity in these bands are main-sequence turnoff stars and giants. Our results on the colours and M/L for the ‘solar cylinder’ well agree with population synthesis predictions using initial mass functions typical of the solar neighbourhood. Finally, we infer the global luminosity of the Milky Way, which appears to be underluminous by about 1σ with respect to the main locus of the Tully–Fisher relation, as observed for external galaxies.
AbstractList ABSTRACT We measure the volume luminosity density and surface luminosity density generated by the Galactic disc, using accurate data on the local luminosity function and the vertical structure of the disc. From the well‐measured volume mass density and surface mass density, we derive local volume and surface mass‐to‐light ratios (M/L) for the Galactic disc, in the bands B, V and I. We obtain M/L for the local column of stellar matter of (M/L)B= 1.4 ± 0.2, (M/L)V= 1.5 ± 0.2 and (M/L)I= 1.2 ± 0.2. The dominant contributors to the surface luminosity in these bands are main‐sequence turnoff stars and giants. Our results on the colours and M/L for the ‘solar cylinder’ well agree with population synthesis predictions using initial mass functions typical of the solar neighbourhood. Finally, we infer the global luminosity of the Milky Way, which appears to be underluminous by about 1σ with respect to the main locus of the Tully–Fisher relation, as observed for external galaxies.
We measure the volume luminosity density and surface luminosity density generated by the Galactic disc, using accurate data on the local luminosity function and the vertical structure of the disc. From the well-measured volume mass density and surface mass density, we derive local volume and surface mass-to-light ratios (M /L ) for the Galactic disc, in the bands B , V and I. We obtain M /L for the local column of stellar matter of (M/L)B = 1.4 +/- 0.2, (M/L)V = 1.5 +/- 0.2 and (M/L)I = 1.2 +/- 0.2. The dominant contributors to the surface luminosity in these bands are main-sequence turnoff stars and giants. Our results on the colours and M /L for the 'solar cylinder' well agree with population synthesis predictions using initial mass functions typical of the solar neighbourhood. Finally, we infer the global luminosity of the Milky Way, which appears to be underluminous by about 1[tau] with respect to the main locus of the Tully-Fisher relation, as observed for external galaxies. [PUBLICATION ABSTRACT]
We measure the volume luminosity density and surface luminosity density generated by the Galactic disc, using accurate data on the local luminosity function and the vertical structure of the disc. From the well-measured volume mass density and surface mass density, we derive local volume and surface mass-to-light ratios (M/L) for the Galactic disc, in the bands B, V and I. We obtain M/L for the local column of stellar matter of (M/L) B = 1.4 ± 0.2, (M/L) V = 1.5 ± 0.2 and (M/L) I = 1.2 ± 0.2. The dominant contributors to the surface luminosity in these bands are main-sequence turnoff stars and giants. Our results on the colours and M/L for the 'solar cylinder' well agree with population synthesis predictions using initial mass functions typical of the solar neighbourhood. Finally, we infer the global luminosity of the Milky Way, which appears to be underluminous by about 1σ with respect to the main locus of the Tully-Fisher relation, as observed for external galaxies.
We measure the volume luminosity density and surface luminosity density generated by the Galactic disc, using accurate data on the local luminosity function and the vertical structure of the disc. From the well-measured volume mass density and surface mass density, we derive local volume and surface mass-to-light ratios (M/L) for the Galactic disc, in the bands B, V and I. We obtain M/L for the local column of stellar matter of (M/L)B= 1.4 ± 0.2, (M/L)V= 1.5 ± 0.2 and (M/L)I= 1.2 ± 0.2. The dominant contributors to the surface luminosity in these bands are main-sequence turnoff stars and giants. Our results on the colours and M/L for the ‘solar cylinder’ well agree with population synthesis predictions using initial mass functions typical of the solar neighbourhood. Finally, we infer the global luminosity of the Milky Way, which appears to be underluminous by about 1σ with respect to the main locus of the Tully–Fisher relation, as observed for external galaxies.
Author Fuchs, Burkhard
Jahreiß, Hartmut
Holmberg, Johan
Flynn, Chris
Portinari, Laura
Author_xml – sequence: 1
  givenname: Chris
  surname: Flynn
  fullname: Flynn, Chris
  email: cflynn@astro.utu.fi, cflynn@astro.utu.fi
  organization: Tuorla Observatory, Väisäläntie 20, FI-21500 Piikkiö, Finland
– sequence: 2
  givenname: Johan
  surname: Holmberg
  fullname: Holmberg, Johan
  organization: Tuorla Observatory, Väisäläntie 20, FI-21500 Piikkiö, Finland
– sequence: 3
  givenname: Laura
  surname: Portinari
  fullname: Portinari, Laura
  organization: Tuorla Observatory, Väisäläntie 20, FI-21500 Piikkiö, Finland
– sequence: 4
  givenname: Burkhard
  surname: Fuchs
  fullname: Fuchs, Burkhard
  organization: Astronomisches Rechen-Institut am Zentrum für Astronomie der Universität Heidelberg, Mönchhofstrasse 12-14, Heidelberg, Germany
– sequence: 5
  givenname: Hartmut
  surname: Jahreiß
  fullname: Jahreiß, Hartmut
  organization: Astronomisches Rechen-Institut am Zentrum für Astronomie der Universität Heidelberg, Mönchhofstrasse 12-14, Heidelberg, Germany
BackLink http://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=18204845$$DView record in Pascal Francis
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10.1086/308700
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Sun Oct 22 16:07:46 EDT 2023
Sat Aug 24 00:55:13 EDT 2024
Wed Sep 11 04:49:37 EDT 2024
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Issue 3
Keywords galaxies: fundamental parameters
Galaxy: disc
Mass to light ratio
Color
Disk galaxies
Tully Fisher relation
Luminosity
Main sequence stars
Galactic disks
Milky Way
Solar neighborhood
Initial mass function
Cylinders
Luminosity function
Language English
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Snippet We measure the volume luminosity density and surface luminosity density generated by the Galactic disc, using accurate data on the local luminosity function...
ABSTRACT We measure the volume luminosity density and surface luminosity density generated by the Galactic disc, using accurate data on the local luminosity...
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SubjectTerms Astronomy
Earth, ocean, space
Exact sciences and technology
galaxies: fundamental parameters
Galaxy: disc
Luminosity
Milky Way
Stars & galaxies
Title On the mass-to-light ratio of the local Galactic disc and the optical luminosity of the Galaxy
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