The Magellanic Clouds
A multifrequency study of the Magellanic Clouds
... the Magellanic Clouds 775 PN sample brighter than the LMC? Could we be missing even more brighter LMC ones? However, the existence of the observable infrared emission for the four of the five detected SMC ...
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Radio Pulsars in the Magellanic Clouds
... using this receiver to search for pulsars in the Galactic plane, and that survey has discovered 580 pulsars to date (Camilo et al. 2000a; Manchester et al. 2000; Lyne et al. 2000). This demonstrates that the multibeam ...
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Radio Pulsars in the Magellanic Clouds
... Small Magellanic Cloud (SMC) for radio pulsars conducted with the 20 cm multibeam receiver of the Parkes 64 m ...Large Magellanic Cloud ...the Magellanic Clouds to ...luminous ...
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Star cluster evolution in the Magellanic Clouds revisited
... the Magellanic Clouds are as yet the best available calibrators for the canonical young CLFs that form the basis of most theoretical attempts to explain the evolution of the CLF and ...the Magellanic ...
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Chemical evolution of the Magellanic Clouds: analytical models
... Accepted 1998 May 6. Received 1998 May 6; in original form 1998 January 26 A B S T R A C T We have extended our analytical chemical evolution modelling ideas for the Galaxy to the Magellanic Clouds. Unlike ...
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PLANETARY NEBULAE AND THE CHEMICAL EVOLUTION OF THE MAGELLANIC CLOUDS
... the Magellanic Clouds, so that we can obtain re- liable constraints on the nucleosynthesis processes in the progenitor stars in galaxies of different ...
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Discovery of 14 Radio Pulsars in a Survey of the Magellanic Clouds
... s: Magellanic Clouds — pulsars: general — surveys Online material: color figures ...Small Magellanic Clouds ( LMC and SMC) are our nearest neighbor galaxies and, to date, the only galaxies ...
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Discovery of 14 radio pulsars in a survey of the Magellanic Clouds
... for the Galactic population) and the largest (for PSR J0543−6851) is only 0.082. Only two pulsars, PSRs J0543−6851 and J0555−7056, have clear evidence for multiple components in the mean profile. Five of the seven ...
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IR imaging surveys of AGB stars in the Magellanic Clouds
... the Magellanic Bridge and of the LMC at ∼ 4 kpc from its centre supporting tidal stripping resulting from the dynamical interaction between the Magellanic ...
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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 ...
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Structure, Abundances, and Reddening of the Magellanic Clouds from its Variable Stars
... the Magellanic Clouds. The depth extend of both Clouds is significant, with ∼ 2 kpc for the Large Magellanic Cloud and a Small Magellanic Cloud depth of ∼ 4 ...Large Magellanic ...
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The VISTA near-infrared YJKs public survey of the Magellanic Clouds System (VMC)
... the Magellanic Clouds System (VMC) Cioni, M R ; Clementini, G ; et al Abstract: The VISTA public survey project VMC targets the Large Magellanic Cloud, the Small Mag- ellanic Cloud, the Bridge and ...
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The structure of the Magellanic Clouds traced by red clump stars at near-infrared wavelengths
... finding that the bar initially had a low activity followed by an enhancement in the star formation rate that occurred 4–6 Gyr ago which has remained fairly constant since. The timing of this enhancement is thought to be ...
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Results of the ESO-SEST key programme: CO in the Magellanic Clouds. VI. The 30 DOR Complex
... molecular clouds in a complex extending ∼ 2 kpc south of 30 Dor in the Large Magellanic ...22 clouds whose sizes and line profiles look like that from Milky Way molecular ...
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The star formation history of the Magellanic Clouds derived from long-period variable star counts
... – Magellanic Clouds – galaxies: star formation – galaxies: stellar content – galaxies: ...The Magellanic Clouds (Large, LMC, and Small, SMC) are irregu- lar, gas-rich dwarf galaxies in our ...
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An atlas of cool supergiants from the Magellanic Clouds and typical interlopers. A guide for the classification of luminous red stars
... We present an atlas composed of more than 1500 spectra of late-type stars (spectral types from G to M) observed simultaneously in the optical and calcium triplet spectral ranges. These spectra were obtained as part of a ...
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First constraints on the magnetic field strength in extra-Galactic stars: FORS2 observations of Of?p stars in the Magellanic Clouds
... We know that the Magellanic Clouds (MCs) host chemi- cally peculiar stars ( Maitzen et al. 2001 ; Paunzen et al. 2011 ), but they are too faint to be checked for magnetic fields with the currently available ...
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The Contribution of Thermally-Pulsing Asymptotic Giant Branch and Red Supergiant Starts to the Luminosities of the Magellanic Clouds at 1-24 micrometers
... The large mid-IR TP-AGB contributions predicted by these previous works (e.g., >50% of the 8 and 24 μm flux) likely arose from their adopted mid-IR colors and fluxes of C-AGB stars. Kelson & Holden ( 2010 ) and ...
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Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds. X. CO emission from star formation regions in LMC and SMC
... galaxies: Magellanic Clouds – galaxies: ISM – galaxies: irregular – galaxies: Local Group – ISM: molecules ...the Magellanic Clouds. It was noted that the Magellanic Clouds allow ...
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Sasaki, Manami (2002): X-rays tracing the star formation history of the Magellanic clouds. Dissertation, LMU München: Fakultät für Physik
... the Magellanic Clouds has been ...the Magellanic Clouds in the soft X-ray band and by analyzing the hot component of the interstellar ...
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