Results 71 to 80 of about 553 (184)
The period distribution of Cepheids: a test of stellar evolution
EPJ Web of Conferences, 2015 The period distributions of classical Cepheids in the Small and Large Magellanic Cloud are quite different. Using the TRILEGAL population synthesis code and a theoretical instability strip the ultimate aim is to understand these differences ...
Groenewegen M.A.T., Girardi L.
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Dark matter annihilations in the Large Magellanic Cloud [PDF]
Nuclear Physics B - Proceedings Supplements, 1994 2pp, plain TeX ...
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SPECTRAL LINE SURVEY TOWARD MOLECULAR CLOUDS IN THE LARGE MAGELLANIC CLOUD [PDF]
The Astrophysical Journal, 2016 ABSTRACT Spectral line survey observations of seven molecular clouds in the Large Magellanic Cloud (LMC) have been conducted in the 3 mm band with the Mopra 22 m telescope to reveal chemical compositions in low metallicity conditions. Spectral lines of fundamental species such as CS, SO, CCH, HCN, HCO+, and HNC are detected in addition ...
Yuri Nishimura +6 more
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The Astronomical JournalSupergiant shells (SGSs) are the largest interstellar structures where heated and enriched gas flows into the host galaxy’s halo. The SGSs in the Large Magellanic Cloud (LMC) are so close that their stars can be resolved with ground-based telescopes to ...
Po-Sheng Ou +4 more
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COSMIC RAY ACCELERATORS IN THE LARGE MAGELLANIC CLOUD [PDF]
The Astrophysical Journal, 2010 I point out a correlation between gamma-ray emissivity and the historical star formation rate in the Large Magellanic Cloud ~12.5 Myr ago. This correlation bolsters the view that CRs in the LMC are accelerated by conglomerations of supernova remnants: i.e. superbubbles and supergiant shells.
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The Large Magellanic Cloud R Crb Star — HV12842 [PDF]
International Astronomical Union Colloquium, 1985 The star HV12842 is one of the 5 R CrB stars listed in the catalogue of variable stars in the LMC (Payne-Goposchkin 1971) and is located 4 deg. to the north of 30 Doradus. At this location it falls in the north-eastern part of one of two standard LMC fields used by the UK 1.2 m Schmidt Telescope.
D.H. Morgan, K. Nandy, N. Kameswara Rao
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Properties of the Magellanic Corona
The Astrophysical JournalWe characterize the Magellanic Corona, the warm gaseous halo around the Large Magellanic Cloud (LMC). The Corona is a key ingredient in the formation of the Magellanic Stream and has recently been observed in high-ion absorption around the LMC.
Scott Lucchini +2 more
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Large Magellanic Cloud Cepheids in the ASAS data
Acta Astronomica, 2011 A catalog of Cepheids in the Large Magellanic Cloud (LMC) from the ASAS project is presented. It contains data on 65 fundamental mode pulsators with periods longer than about 8 days. The period-luminosity (PL) relation in the V-band does not significantly differ from the relation determined by Soszynski et al.
Karczmarek, P +4 more
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The Large Magellanic Cloud and the distance scale [PDF]
Astrophysics and Space Science, 2011 23 pages, accepted for publication in Astrophysics and Space Science. From a presentation at the conference The Fundamental Cosmic Distance Scale: State of the Art and the Gaia Perspective, Naples, May ...
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The Astrophysical JournalIn this work, we present spectra of 11 young stellar objects (YSOs) taken with the Mid-Infrared Instrument / Medium Resolution Spectroscopy (MRS) instrument on board the James Webb Space Telescope (JWST).
Omnarayani Nayak +11 more
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