The Large Magellanic Cloud
Infrared composition of the Large Magellanic Cloud
... Srinivasan, S., B. A. Sargent, and M. Meixner, The mass-loss return from evolved stars to the Large Magellanic Cloud. V. The GRAMS carbon- star model grid, Astron. Astrophys., 532, A54, 2011. ...
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CiteSeerX — The Proper Motion of the Large Magellanic Cloud: A Reanalysis
... the Large Magellanic Cloud (LMC) relative to four background quasi-stellar objects, combining data from two previous studies made by our group, and new observations carried out in four epochs not ...
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Eight New Radio Pulsars in the Large Magellanic Cloud
... the Large Magellanic Cloud ...the Magellanic Clouds, while the remaining three were from an ongoing new survey at Parkes with a high-resolution data acquisition ...the large number of ...
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A survey for stellar relics of galaxy formation in the large Magellanic cloud
... We aim to identify some of the first extremely metal-poor stars in the Large Magellanic Cloud (LMC) based on photometric selection of red giants. The pho- tometric data were from observations using ...
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The VMC survey – XXXVI. Young stellar variability in the Large Magellanic Cloud
... the Large Magellanic Cloud ...the Magellanic Clouds (VMC) and our own monitoring campaign using the VISTA ...two Magellanic YSOs exhibit Ks > 1 mag), not what would have been ...
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The (non-)variability of magnetic chemically peculiar candidates in the Large Magellanic Cloud
... http://www.aanda.org of sight. The observed amplitudes are up to a few tenths of magnitudes. However, for some stars one also fails to find any rotational induced variability at all. The locations of spots used to have ...
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An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent
... 9. Graczyk, D., et al. The Araucaria Project. An Accurate Distance to the Late-type Double-lined Eclipsing Binary OGLE SMC113.3 4007 in the Small Magellanic Cloud. Astrophys. J., 750, 144-156 (2012) 10. ...
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Star-density Profiles of Six Old Star Clusters in the Large Magellanic Cloud
... Abstract We used resolved star counts from Hubble Space Telescope (HST) images to determine the center of gravity and the projected density pro files of six old globular clusters (GCs) in the Large ...
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Deep Washington photometry of inconspicuous star cluster candidates in the Large Magellanic Cloud
... ABSTRACT We present deep Washington photometry of 45 poorly populated star cluster candidates in the Large Magellanic Cloud (LMC). We have performed a systematic study to estimate the parameters of ...
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Deep Washington photometry of inconspicuous star cluster candidates in the Large Magellanic Cloud
... We present deep Washington photometry of 45 poorly populated star cluster candidates in the Large Magellanic Cloud (LMC). We have performed a systematic study to estimate the parameters of the ...
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Variability of Luminous Stars in the Large Magellanic Cloud Using 10 Years of ASAS Data
... 4 Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, USA; [email protected] Received 2010 February 1; accepted 2010 April 20; published 2010 May 18 ABSTRACT Motivated by the detection of a ...
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Absolute parameters for eight eclipsing binaries in the Large Magellanic Cloud: The mass-luminosity relation
... eight Large Magellanic Cloud (LMC) eclipsing binaries is ...Very Large Telescope and light curves available from the MACHO and OGLE databases, accurate masses and radii for the binary ...
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Accurate radial velocity and metallicity of the Large Magellanic Cloud old globular clusters NGC1928 and NGC1939
... 5 Laborat´ orio Nacional de Astrof´ısica, R. Estados Unidos 154, 37530-000 Itajub´ a, MG, Brazil Accepted XXX. Received YYY; in original form ZZZ ABSTRACT We present results obtained from spectroscopic observations of ...
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Eclipsing binaries in the MACHO database: New periods and classifications for 3031 systems in the Large Magellanic Cloud
... Eclipsing binaries offer a unique opportunity to determine fundamental physical parameters of stars using the constraints on the geometry of the systems. Here we present a reanalysis of publicly available two-color ...
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Variability of the pulsed radio emission from the large magellanic cloud pulsar PSR J0529–6652
... Generally, m is observed to be small, with typical values between about 0.5 and 1 (Weltevrede et al. 2006a , 2011 ; Burke- Spolaor et al. 2012 ). The histogram of measured modulation indices shown in Figure 8 of ...
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Spitzer Space Telescope spectra of post AGB stars in the large magellanic Cloud polycyclic aromatic hydrocarbons at low metallicities
... A B S T R A C T This paper reports variations of polycyclic aromatic hydrocarbons (PAHs) features that were found in Spitzer Space Telescope spectra of carbon-rich post-asymptotic giant branch (post- AGB) stars in the ...
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Polarisation in the galaxy and the large Magellanic Cloud
... in the Aust:celian Natiol~al University Canberra.. Tilting the po l 'rime~er. Reduction of datG-.. Calcule tion of external errors .... Interpl'etation of our results ... [r] ...
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The evolution of HII regions in the Large Magellanic Cloud
... Dopita's model has a stellar wind bubble being formed by mass-loss from an OB star (or stars) located off-centre in a large collapsing9. molecular cloud.[r] ...
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The Master Catalogue of stars towards the Magellanic Clouds. I. Multispectral surveys of the Large Magellanic Cloud
... the Magellanic Clouds (MC2) is a multi–wavelength reference ...the Magellanic Clouds (DCMC) with more than ...the Magellanic Clouds ...very large catalogues have been developed and important ...
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The nature and kinematics of long-period variables in the Large Magellanic Cloud
... a large subsample of the now almost complete search for LPVs in the ...as large amplitude pulsators than do LPVs in the Galaxy, probably because the lower metallicity of the LMC means th a t a large ...
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