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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 660902.0, MPI für Astronomie / Publikationen_mpia
The present-day mass function of the Quintuplet cluster based on proper motion membership
Authors:Hußmann, B.; Stolte, A.; Brandner, W.; Gennaro, M.; Liermann, A.
Date of Publication (YYYY-MM-DD):2012
Title of Journal:Astronomy and Astrophysics
Journal Abbrev.:A & A
Volume:540
Start Page:id. A57
Review Status:not specified
Audience:Not Specified
Abstract / Description:Context. The stellar mass function is a probe for a potential dependence of star formation on the environment. Only a few young clusters are known to reside within the central molecular zone and can serve as testbeds for star formation under the extreme conditions in this region. <BR /> Aims: We determine the present-day mass function of the Quintuplet cluster, a young massive cluster in the vicinity of the Galactic centre. <BR /> Methods: We use two epochs of high resolution near infrared imaging data obtained with NAOS/CONICA at the ESO VLT to measure the individual proper motions of stars in the Quintuplet cluster in the cluster reference frame. An unbiased sample of cluster members within a radius of 0.5 pc from the cluster centre was established based on their common motion with respect to the field and a subsequent colour-cut. Initial stellar masses were inferred from four isochrones covering ages from 3 to 5 Myr and two sets of stellar evolution models. For each isochrone, the present-day mass function of stars was determined for the full sample of main sequence cluster members using an equal number binning scheme. <BR /> Results: We find the slope of the present-day mass function in the central part of the Quintuplet cluster to be α = -1.68+0.13-0.09, which is significantly flatter than the Salpeter slope of α = -2.35. The flattening of the present-day mass function may be caused by rapid dynamical evolution of the cluster in the strong Galactic centre tidal field. The derived mass function slope is compared to the values found in other young massive clusters in the Galaxy. Based on observations collected at the ESO/VLT under Program ID 71.C-0344(A) (PI: F. Eisenhauer, retrieved from the ESO archive) and Program ID 081.D-0572(B) (PI: W. Brandner).Appendices are available in electronic form at <A href="http://www.aanda.org">http://www.aanda.org</A>Full Table 4 is available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/540/A57">http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/540/A57</A>
Free Keywords:Galaxy: center; open clusters and associations: individual: Quintuplet cluster; stars: early-type; infrared: stars; stars: luminosity function; mass function; stars: kinematics and dynamics
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://cdsads.u-strasbg.fr/abs/2012A%26A...540A..5... [ID No:1]
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