Large Magellanic Cloud
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 nature and kinematics of long-period variables in the Large Magellanic Cloud
... the Large Magellanic Cloud (LMC) using red-sensitive I plates have been carried out by Reid, Glass & Catchpole (1987; hereinafter RGC) and in Chapter ...
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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 ...
10
Variability of Luminous Stars in the Large Magellanic Cloud Using 10 Years of ASAS Data
... stars in the Large Magellanic Cloud, using a recent catalog by Bonanos et al. as the input. The ASAS All Star Catalog provided well-sampled light curves of these bright stars spanning 10 years. ...
11
Polarisation in the galaxy and the large Magellanic Cloud
... Considering that the pola ris a tion due to our Galaxy, in the field of Larg e Magellanic Cloud is less than 0.002 mag and that for the Cloud stars the mean error in the determination of[r] ...
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The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud
... The MLRs of the four stars turn out to be very similar and in agreement with the MLRs found for the Galactic extreme C- stars. When plotted against luminosity there is one obvious out- lier, ERO 0529379. Its luminosity ...
11
Milky way halo objects, IC 4499 and the large magellanic cloud
... recent Magellanic histories show that LMC-SMC close encounters over the last 2 Gyr, in addition to an approaching MW, can trigger patchy star formation in the LMC along the bar and regions like 30 Do- radus (Bekki ...
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No compelling evidence of significant early star cluster disruption in the Large Magellanic Cloud
... mation history based on CMD analysis (for a recent discussion, see Maschberger & Kroupa 2011), provided that the star and cluster formation histories can be mapped on to one another within reason- ably small ...
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Star cluster formation history along the minor axis of the Large Magellanic Cloud
... few new star cluster candidates detected would not appear to sup- port some recent outcomes which have shown that there are still a substantial number of extreme low luminosity stellar clusters unde- tected in the wider ...
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Thermal and Non-Thermal Contributions to the X-ray Spectrum of Large Magellanic Cloud Supernova Remnants
... As discussed above, single-component NEI models assume a single temperature and single ionization timescale for the emitting plasma. The HE model should be able to reproduce the behavior of NEI models for large τ ...
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Accurate radial velocity and metallicity of the Large Magellanic Cloud old globular clusters NGC1928 and NGC1939
... Only stars #1 and 6 observed in the field of NGC 1939 have RV memberships different from those adopted using separately their positions in the cluster CMDs and their metallicities, respe[r] ...
10
Infrared composition of the Large Magellanic Cloud
... With Spitzer it became possible to obtain 5–40 μm spec- troscopy of many point sources in the LMC and SMC. In- deed, many observing programs were proposed, some tar- geting just a single or a few point sources, while ...
5
The evolution of HII regions in the Large Magellanic Cloud
... together with the hydrogen-alpha surface photometry, are used to show that the large shell-like HII regions in the L.M.C. are stellar wind bubbles 3 to 5 million years old. In order to reproduce the observed ...
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The Master Catalogue of stars towards the Magellanic Clouds. I. Multispectral surveys of the Large Magellanic Cloud
... of large surveys is, to derive results on their internal ...the large number of sources involved, al- low a multi–wavelength and statistical study of the stellar pop- ulations of the ...
13
Properties of Anomalous and Type II Cepheids in the Small and Large Magellanic Clouds
... Small Magellanic Cloud (SMC) and Large Magellanic Cloud (LMC) give us the possibility to study individual variable star types in a new ...
5
A multi-frequency analysis of radio supernova remnants and their environments in Sculptor Group SD Galaxy NGC 300 and the Small Magellanic Cloud
... of Large Magellanic Cloud radio supernova remnants”, published in the Monthly Notices of the Royal Astronomical Society (MNRAS), 2008, volume 383, pages ...
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Storage of Flexible and Large Data in Cloud Computing
... in Cloud Computing International Journal of Advanced Technology and Innovative Research Subsequently, we present the AnonyControl F, which fully prevents the identity leakage and achieve the full ...
8
Challenges of Cloud Solutions Adoption in Large Corporations
... and cloud systems is a major challenge in a hybrid cloud ...practice cloud implementations, it is highly recommended to use a middleware as an Enterprise Service Bus (ESB) to implement integration ...
5
Simulation of a Large Scaled Web Application on the Cloud Using Cloud Analyst
... the Cloud can use this tool to perform some benchmarking experiments with the services to be offered in dependable, scalable, repeatable, and controllable environments before real deployment in the ...
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A multi-frequency analysis of radio supernova remnants and their environments in Sculptor Group SD Galaxy NGC 300 and the Small Magellanic Cloud
... Chapter 3, originally entitled, “An ATCA radio-continuum study of the Small Magellanic Cloud - II. Source identification and classification” was published in 2004 by the Monthly Notices of the Royal Astro- ...
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