The LMC Geometry and Outer Stellar Populations from Early DES Data
- Univ. of Surrey, Guildford (United Kingdom); Universidade Federal do Rio Grande do Sul, Porto Alegre (Brazil); Laboratorio Interinstitucional de e-Astronomia, Rio de Janerio (Brazil)
- Universidade Federal do Rio Grande do Sul, Porto Alegre (Brazil); Laboratorio Interinstitucional de e-Astronomia, Rio de Janerio (Brazil)
- Osservatorio Astronommic di Padova INAF (Italy)
- Laboratorio Interinstitucional de e-Astronomia and Observatorio Nacional, Rio de Janerio (Brazil)
- Univ. of Illinois, Urbana, IL (United States)
- National Optical Astronomy Observatory, La Serena (Chile)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Univ. College London (United Kingdom)
- Argonne National Lab. (ANL), Argonne, IL (United States)
- Carnegie Observatories, Pasadena, CA (United States)
- Univ. Pierre et Marie Curie, Paris (France)
- Stanford Univ., CA (United States)
- Texas A & M Univ., College Station, TX (United States)
- Ludwig Maximilian Univ., Munich (Germany); Excellence Cluster Universe, Garching (Germany)
- Laboratorio Interinstitucional de e-Astronomia, Rio de Janerio (Brazil)
- Ludwig Maximilian Univ., Munich (Germany); Max Planck Inst. for Extraterrestrial Physics, Garching (Germany)
- The Ohio State Univ., Columbus, OH (United States)
- Australian Astronomical Observatory, North Ryde (Australia)
- Univ. of Pennsylvania, Philadelphia, PA (United States)
- Univ. of Michigan, Ann Arbor, MI (United States)
- Univesitat Autonoma de Barcelona (Spain); Institucio Catalana de Recerca i Estudis Avancats, Barcelona (Spain)
- Brookhaven National Lab. (BNL), Upton, NY (United States)
- Medioambientales y Tecnologicas (CIEMAT), Madrid (Spain)
- Excellence Cluster Universe, Garching (Germany); SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Univ. of Manchester (United Kingdom)
The Dark Energy Camera has captured a large set of images as part of Science Verification (SV) for the Dark Energy Survey. The SV footprint covers a large portion of the outer Large Magellanic Cloud (LMC), providing photometry 1.5 magnitudes fainter than the main sequence turn-off of the oldest LMC stellar population. We derive geometrical and structural parameters for various stellar populations in the LMC disc. For the distribution of all LMC stars, we find an inclination of i = –38.14°±0.08° (near side in the North) and a position angle for the line of nodes of θ₀ = 129.51°±0.17°. We find that stars younger than ~4 Gyr are more centrally concentrated than older stars. Fitting a projected exponential disc shows that the scale radius of the old populations is R>4Gyr = 1.41 ± 0.01 kpc, while the younger population has R<4Gyr = 0.72 ± 0.01 kpc. However, the spatial distribution of the younger population deviates significantly from the projected exponential disc model. The distribution of old stars suggests a large truncation radius of Rt = 13.5 ± 0.8 kpc. If this truncation is dominated by the tidal field of the Galaxy, we find that the LMC is ≃24+9–6 times less massive than the encircled Galactic mass. By measuring the Red Clump peak magnitude and comparing with the best-fit LMC disc model, we find that the LMC disc is warped and thicker in the outer regions north of the LMC centre. As a result, our findings may either be interpreted as a warped and flared disc in the LMC outskirts, or as evidence of a spheroidal halo component.
- Research Organization:
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Brookhaven National Laboratory (BNL), Upton, NY (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Organization:
- DES Collaboration
- Grant/Contract Number:
- AC02-07CH11359; SC00112704; AC02-76SF00515
- OSTI ID:
- 1226324
- Alternate ID(s):
- OSTI ID: 1201363; OSTI ID: 1510826
- Report Number(s):
- FERMILAB-PUB-15-045-AE; BNL-108183-2015-JA; arXiv eprint number arXiv:1502.05050
- Journal Information:
- Monthly Notices of the Royal Astronomical Society (Online), Vol. 449, Issue 1; ISSN 1365-2966
- Publisher:
- Royal Astronomical SocietyCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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