Works matching IS 17439213 AND DT 2008 AND VI 4 AND IP S256
Results: 68
The Magellanic System: Stars, Gas, and Galaxies.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 489, doi. 10.1017/S1743921308028913
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Evidence of Magellanic-like moderate redshift H i-rich galaxies.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 479, doi. 10.1017/S1743921308028895
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The Magellanic Group and the Seven Dwarfs.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 473, doi. 10.1017/S1743921308028883
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The optically bright post-AGB population of the LMC.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 415, doi. 10.1017/S1743921308028809
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Dust around red supergiants in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 411, doi. 10.1017/S1743921308028792
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Magellanic type galaxies throughout the Universe.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 461, doi. 10.1017/S1743921308028871
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High-exitation nebulae around Magellanic Wolf-Rayet stars.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 437, doi. 10.1017/S1743921308028834
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On the huge mass loss of B[e] supergiants in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 431, doi. 10.1017/S1743921308028822
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The population of Magellanic Cloud planetary nebulae.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 421, doi. 10.1017/S1743921308028810
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Resolving the dusty torus and the mystery surrounding LMC red supergiant WOH G64.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 454, doi. 10.1017/S1743921308028858
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Supernova remnants in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 443, doi. 10.1017/S1743921308028846
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The production of dust in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 405, doi. 10.1017/S1743921308028780
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A study of AGB stars in LMC clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 397, doi. 10.1017/S1743921308028767
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A comprehensive study of the link between star-formation history and X-ray source populations in the SMC.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 355, doi. 10.1017/S1743921308028706
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Thermally-pulsing asymptotic giant branch stars in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 385, doi. 10.1017/S1743921308028743
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Pulsating variable stars in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 373, doi. 10.1017/S1743921308028731
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Optical properties of High-Mass X-ray Binaries (HMXBs) in the Small Magellanic Cloud.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 367, doi. 10.1017/S174392130802872X
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Properties of X-ray binaries in the Magellanic Clouds from RXTE and Chandra observations.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 361, doi. 10.1017/S1743921308028718
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On the self-consistent physical parameters of LMC intermediate-age clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 391, doi. 10.1017/S1743921308028755
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The WFI Hα spectroscopic survey of the Magellanic Clouds: Be stars in SMC open clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 349, doi. 10.1017/S174392130802869X
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Multiple stellar populations in massive LMC star clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 305, doi. 10.1017/S1743921308028627
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Stellar evolution models at the Magellanic Cloud metallicities.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 337, doi. 10.1017/S1743921308028676
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The properties of early-type stars in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 325, doi. 10.1017/S1743921308028664
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Gemini/GMOS detection of stellar velocity variations in the ionising cluster of 30 Dor.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 317, doi. 10.1017/S1743921308028640
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Star cluster evolution in the Magellanic Clouds revisited.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 311, doi. 10.1017/S1743921308028639
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A survey of the most massive stars in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 343, doi. 10.1017/S1743921308028688
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The chemical signatures of the Large Magellanic Cloud globular clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 299, doi. 10.1017/S1743921308028615
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Integrated spectral properties of star clusters in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 293, doi. 10.1017/S1743921308028603
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Metallicity and kinematics of a large sample of LMC and SMC clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 287, doi. 10.1017/S1743921308028597
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Spatial variations in the star formation history of the Large Magellanic Cloud.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 281, doi. 10.1017/S1743921308028585
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The chemical enrichment history of the Magellanic Clouds field populations.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 275, doi. 10.1017/S1743921308028573
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The star formation history in 12 SMC fields.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 269, doi. 10.1017/S1743921308028561
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Breaking the age–metallicity degeneracy: The metallicity distribution and star formation history of the Large Magellanic Cloud.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 263, doi. 10.1017/S174392130802855X
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An observational study of GMCs in the Magellanic Clouds with the ASTE telescope.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 256, doi. 10.1017/S1743921308028536
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The properties of molecular clouds across the Magellanic System.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 203, doi. 10.1017/S1743921308028469
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The sub-solar initial mass function in the Large Magellanic Cloud.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 250, doi. 10.1017/S1743921308028524
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Insights from Spitzer on massive star formation in the LMC.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 239, doi. 10.1017/S1743921308028500
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AKARI near-infrared spectroscopy: Detection of H2O and CO2 ices toward young stellar objects in the Large Magellanic Cloud.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 233, doi. 10.1017/S1743921308028494
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Star-formation masers in the Magellanic Clouds: A multibeam survey with new detections and maser abundance estimates.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 227, doi. 10.1017/S1743921308028482
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Properties of star forming regions in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 215, doi. 10.1017/S1743921308028470
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Time resolved star formation in the SMC: the youngest star clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 244, doi. 10.1017/S1743921308028512
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The star formation process in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 191, doi. 10.1017/S1743921308028457
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Tracing the cold molecular gas reservoir through dust emission in the SMC.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 148, doi. 10.1017/S174392130802838X
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The magnetic field structure of the Small Magellanic Cloud.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 178, doi. 10.1017/S1743921308028421
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The violent interstellar medium of the Magellanic Cloud System.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 166, doi. 10.1017/S174392130802841X
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The Spitzer spectroscopic survey of the Small Magellanic Cloud: polycyclic aromatic hydrocarbon emission from SMC star-forming regions.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 160, doi. 10.1017/S1743921308028408
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The state of molecular gas in the Small Magellanic Cloud.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 154, doi. 10.1017/S1743921308028391
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Early results from the SAGE-SMC Spitzer legacy.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 184, doi. 10.1017/S1743921308028433
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Dust in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 137, doi. 10.1017/S1743921308028378
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The many streams of the Magellanic Stream.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 129, doi. 10.1017/S1743921308028354
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