Searching in the dark: the dark mass content of the Milky Way globular clusters NGC288 and NGC6218

Autor: Alessio Mucciarelli, E. Lapenna, Emanuele Dalessandro, Livia Origlia, Antonio Sollima, Francesco R. Ferraro, C. Pallanca, Barbara Lanzoni, Filippo Contenta, Enrico Vesperini, L. Lovisi
Přispěvatelé: Sollima, A., Ferraro, F.R., Lovisi, L., Contenta, F., Vesperini, E., Origlia, L., Lapenna, E., Lanzoni, B., Mucciarelli, A., Dalessandro, E., Pallanca, C., ITA, USA, GBR
Rok vydání: 2016
Předmět:
Astrophysics::High Energy Astrophysical Phenomena
Milky Way
FOS: Physical sciences
Tidal heating
Stars: luminosity function
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
01 natural sciences
0103 physical sciences
Cluster (physics)
Astrophysics::Solar and Stellar Astrophysics
010303 astronomy & astrophysics
Solar and Stellar Astrophysics (astro-ph.SR)
Astrophysics::Galaxy Astrophysics
Physics
Techniques: radial velocitie
010308 nuclear & particles physics
NGC288
Astronomy
Astronomy and Astrophysics
Stars: kinematics and dynamic
Astronomy and Astrophysic
Astrophysics - Astrophysics of Galaxies
Globular clusters: individual: NGC6218
Stars
Astrophysics - Solar and Stellar Astrophysics
Stars: Population II
Space and Planetary Science
Mass content
Astrophysics of Galaxies (astro-ph.GA)
Mass function
Globular cluster
Dark galaxy
Methods: data analysi
Zdroj: Monthly Notices of the Royal Astronomical Society. 462:1937-1951
ISSN: 1365-2966
0035-8711
DOI: 10.1093/mnras/stw1779
Popis: We present an observational estimate of the fraction and distribution of dark mass in the innermost region of the two Galactic globular clusters NGC 6218 (M12) and NGC 288. Such an assessment has been made by comparing the dynamical and luminous mass profiles derived from an accurate analysis of the most extensive spectroscopic and photometric surveys performed on these stellar systems. We find that non-luminous matter constitutes more than 60% of the total mass in the region probed by our data (R
17 pages, 10 figures, accepted for publication by MNRAS
Databáze: OpenAIRE