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Page 1: AGB Stars in the Magellanic Clouds
Page 2: AGB Stars in the Magellanic Clouds
Page 3: AGB Stars in the Magellanic Clouds
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Gas and dust in the Magellanic clouds

Nature of X-ray transients in the Magellanic Clouds : (Be/X-ray pulsars, and Supersoft sources)

A History of the Magellanic Clouds and the European

Nature of X-ray binaries in the Magellanic Clouds Andry RAJOELIMANANA 1, 2 (MSc) Supervisor : Prof Phil CHARLES 1, 2 1 University of Cape Town, Private

Galaxies next door Mysteries of the Magellanic Clouds/media/Files/PDF/web extras/2011... · The blue and white represents the Milky Way and Magel- lanic Clouds, red is the hydrogen

Modeling dust emission in the Magellanic Clouds with ... · a pixel-by-pixel basis. For example, Roman-Duval et al. (2014) investigated the spatial variations of the GDR in the Magellanic

Nature of High mass X-ray binaries in the Magellanic Clouds Andry RAJOELIMANANA 1, 2 Supervisor : Prof Phil CHARLES 1, 2 Co-supervisor : Prof Brian Warner

The Outer Limits Survey: Stellar Populations at the Extremities of the Magellanic Clouds

Scientific and technical feasibilities of VSOP-2 astrometry of H 2 O masers in the Magellanic Clouds Hiroshi Imai (Kagoshima University) VSOP-2 KSP Maser

Recent Star Formation in the Leading Arm of the Magellanic ... · Milky Way & Environment - Paris, Sept. 2016 D. I. Casetti Magellanic Clouds: The Nearest Gas-rich Galaxy Interaction

THE MAGELLANIC CLOUDS NEWSLETTER

Nature of High mass X-ray binaries in the Magellanic Clouds

Molecular gas and dust in the Magellanic Clouds C. Bot on behalf of Mónica Rubio Dusty, 29 oct 2004

The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turn-offs. I. Results from 19 OB Associations in the Magellanic Clouds

SUPERNOVA REMNANTS IN THE MAGELLANIC CLOUDS JOHN R. DICKEL UNIVERSITY OF NEW MEXICO AND ROSA MURPHY WILLIAMS COLUMBUS STATE UNIVERSITY Preliminary SNR

Galaxies next door Mysteries of the Magellanic Clouds

Nature of X-ray binaries in the Magellanic Clouds

The IRSF Magellanic Clouds Point Source Catalog€¦ · “The IRSF Magellanic Clouds Point Source Catalog” • a NIR point-source catalog for the MCs • covering 55 deg2 of the

Stellar chemistries in dwarf Spheroidal galaxies and the ... · Stellar chemistries in dwarf Spheroidal galaxies and the Magellanic Clouds Vanessa Hill! 1. Stellar chemistries - chemical

Variable stars in the Magellanic Clouds: results from OGLE ...ttanabe/publications/list/... · Mon. Not. R. Astron. Soc. 347, 720–728 (2004) Variable stars in the Magellanic Clouds:

1777 Variables in the Magellanic Clouds-Levitt

SAGE AGB & post-AGB

Authors for “Hubble Space Telescope Observations of Oxygen ...€¦ · Authors for “Hubble Space Telescope Observations of Oxygen-rich Supernova Remnants in the Magellanic Clouds

STAR CLUSTERS IN THE MAGELLANIC CLOUDS - II. AGE-DATING ... · STAR CLUSTERS IN THE MAGELLANIC CLOUDS - II. AGE-DATING, CLASSIFICATION AND SPATIO-TEMPORAL DISTRIBUTION OF THE SMC

The Missing Satellites of the Magellanic Clouds

The Magellanic Clouds and dSph satellites. Vienna, April 10-12

Nature of X-ray transients in the Magellanic Clouds : (Be/X-ray pulsars, and Supersoft sources) Andry RAJOELIMANANA 1, 2 Supervisor : Prof Phil CHARLES

Surveying the Extremities of the Magellanic Clouds A work in progress A. Saha Collaborators: Ed Olszewski Chris Smith Knut Olsen Jason Harris Armin Rest

Submillimeter and IR Studies of Molecular Regions in the Magellanic Clouds Mónica Rubio

A Submillimeter study of the Magellanic Clouds

Supersoft Be X-ray binaries in the Magellanic CloudsSupersoft Be X-ray binaries in the Magellanic Clouds Stefano Ciroi (University of Padova) V. Cracco, M. Orio, J. Gallagher, R. Kotulla,

Polycyclic Aromatic Hydrocarbon from the Magellanic Clouds...Overview 1 Introduction: Polycyclic Aromatic Hydrocarbons Astronomical PAH bands Main interest (tracers, photo-electric

Nearby Galaxies: Templates for Galaxies Across Cosmic Time€¦ · like the Magellanic Clouds provide the best data for understanding how a galaxy’s structure influences the ability

SMASH { SURVEY OF THE MAGELLANIC STELLAR HISTORYdatalab.noao.edu/smash/smash_overview.pdf(SMASH) aims to measure the extended stellar popu-lations of the Clouds and allow us to develop

Star Formation History of the Magellanic Clouds: a survey ...€¦ · evolution; see Figure 2. 5. Enable many community-led projects, including studies involving the LMC/SMC main