Beyond The Brim Of The Hat: Kinematics Of Globular Clusters Out To Large Radii In The Sombrero Galaxy

dc.contributor.utaustinauthorGebhardt, Karlen_US
dc.creatorDowell, Jessica L.en_US
dc.creatorRhode, Katherine L.en_US
dc.creatorBridges, Terry J.en_US
dc.creatorZepf, Stephen E.en_US
dc.creatorGebhardt, Karlen_US
dc.creatorFreeman, Ken C.en_US
dc.creatorde Boer, Elizabeth Wylieen_US
dc.date.accessioned2016-04-22T19:46:34Z
dc.date.available2016-04-22T19:46:34Z
dc.date.issued2014-06en
dc.description.abstractWe have obtained radial velocity measurements for 51 new globular clusters around the Sombrero galaxy. These measurements were obtained using spectroscopic observations from the AAOmega spectrograph on the Anglo-Australian Telescope and the Hydra spectrograph at WIYN. Combining our own past measurements and velocity measurements obtained from the literature, we have constructed a large database of radial velocities that contains a total of 360 confirmed globular clusters. Previous studies' analyses of the kinematics and mass profile of the Sombrero globular cluster system have been constrained to the inner similar to 9' (similar to 24 kpc or similar to 5R(e)), but our new measurements have increased the radial coverage of the data, allowing us to determine the kinematic properties of M104 out to similar to 15' (similar to 41 kpc or similar to 9R(e)). We use our set of radial velocities to study the GC system kinematics and to determine the mass profile and V-band mass-to-light profile of the galaxy. We find that M/L-V increases from 4.5 at the center to a value of 20.9 at 41 kpc (similar to 9R(e) or 15'), which implies that the dark matter halo extends to the edge of our available data set. We compare our mass profile at 20 kpc (similar to 4R(e) or similar to 7.'4) to the mass computed from X-ray data and find good agreement. We also use our data to look for rotation in the globular cluster system as a whole, as well as in the red and blue subpopulations. We find no evidence for significant rotation in any of these samples.en_US
dc.description.departmentAstronomyen_US
dc.description.sponsorshipIndiana Space Grant Consortiumen_US
dc.description.sponsorshipNSF Faculty Early Career Development (CAREER) award AST-0847109en_US
dc.identifierdoi:10.15781/T2S218
dc.identifier.citationDowell, Jessica L., Katherine L. Rhode, Terry J. Bridges, Stephen E. Zepf, Karl Gebhardt, Ken C. Freeman, and Elizabeth Wylie de Boer. >Beyond the Brim of the Hat: Kinematics of Globular Clusters out to Large Radii in the Sombrero Galaxy.> The Astronomical Journal, Vol. 147, No. 6 (Jun., 2014): 150.en_US
dc.identifier.doi10.1088/0004-6256/147/6/150en_US
dc.identifier.issn0004-6256en_US
dc.identifier.urihttp://hdl.handle.net/2152/34449
dc.language.isoEnglishen_US
dc.relation.ispartofserialAstronomical Journalen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.subjectgalaxies: elliptical and lenticular, cden_US
dc.subjectgalaxies: individual (m104)en_US
dc.subjectgalaxies: kinematics and dynamicsen_US
dc.subjectgalaxies: star clusters: generalen_US
dc.subjectx-ray-emissionen_US
dc.subjectwide-fielden_US
dc.subjectkeck spectroscopyen_US
dc.subjectm87 ngc-4486en_US
dc.subjectsystemen_US
dc.subjectdynamicsen_US
dc.subjectngc-4594en_US
dc.subjectphotometryen_US
dc.subjectdistancesen_US
dc.subjectngc-1399en_US
dc.subjectastronomy & astrophysicsen_US
dc.titleBeyond The Brim Of The Hat: Kinematics Of Globular Clusters Out To Large Radii In The Sombrero Galaxyen_US
dc.typeArticleen_US

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