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 |
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Main Authors: | , , , , |
Format: | Journal Article |
Language: | English |
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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. |
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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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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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