نتائج البحث

Molecular and Atomic Gas in the Large Magellanic Cloud. II. Three-dimensional Correlation Between CO and H I

• Authors : Fukui, Y.; Kawamura, A.; Wong, T.

Subjects: galaxies: ISM; ISM: atoms; ISM: clouds

• Source: Astrophysical Journal, 705(1), 144-155, (2009-11-01)

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Molecular and Atomic Gas in the Large Magellanic Cloud. I. Conditions for CO Detection

• Authors : Wong, T.; Hughes, A.; Fukui, Y.

Subjects: galaxies: ISM; ISM: molecules; Magellanic Clouds

• Source: Astrophysical Journal, 696(1), 370-384, (2009-05-01)

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Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5

• Authors : Alsaberi, Rami Z. E.; Maitra, C.; Filipovic, M. D.

Subjects: ISM: INDIVIDUAL OBJECTS: DEMS5; ISM: SUPERNOVA REMNANTS; MAGELLANIC CLOUDS

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Supergiant shells and molecular cloud formation in the large magellanic cloud

• Authors : Dawson, J.R.; McClure-Griffiths, Naomi; Wong, Tony

Subjects: Keywords: evolution; galaxies: ISM; ISM: bubbles

• Source: The Astrophysical Journal

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Early results from the SAGE-SMC Spitzer legacy.

• Authors : Gordon, Karl D.; Meixner, M.; Blum, R. D.

• Source: Proceedings of the International Astronomical Union; 07/02/2008, Vol. 4 Issue S256, p184-188, 5p

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NANTEN observations of triggered star formation: from H II regions to galaxy collisions.

• Authors : Mizuno, N.; Kawamura, A.; Onishi, T.

• Source: Proceedings of the International Astronomical Union; 08/04/2006, Vol. 2 Issue S237, p128-131, 4p

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Giant molecular clouds and star formation in the Large Magellanic Cloud.

• Authors : Kawamura, A.; Minamidani, T.; Mizuno, Y.

• Source: Proceedings of the International Astronomical Union; 08/04/2006, Vol. 2 Issue S237, p101-105, 5p

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Star-Burst Regions in the LMC.

• Authors : Livanou, E.; Kontizas, M.; Gonidakis, I.

• Source: Proceedings of the International Astronomical Union; 08/02/2006, Vol. 2 Issue S235, p318-318, 1p

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Star-Forming Regions in the SMC.

• Authors : Gonidakis, I.; Livanou, E.; Kontizas, E.

• Source: Proceedings of the International Astronomical Union; 08/02/2006, Vol. 2 Issue S235, p311-311, 1p

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