Journal ArticleDOI
Reddenings derived from H I and galaxy counts : accuracy and maps.
D. Burstein,C. Heiles +1 more
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This article is published in The Astronomical Journal.The article was published on 1982-08-01. It has received 1025 citations till now. The article focuses on the topics: Disc galaxy & Interacting galaxy.read more
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A sample of relatively unstudied star clusters in the Large Magellanic Cloud: fundamental parameters determined from Washington photometry
Tali Palma,Tali Palma,Juan J. Clariá,Juan J. Clariá,Doug Geisler,Andrés E. Piatti,Andrea Veronica Ahumada,Andrea Veronica Ahumada +7 more
TL;DR: Palma et al. as discussed by the authors presented a study on the evolution of the Earth's magnetic field using observations from the Observatorio Astronomico de Cordoba (OAC) in Argentina.
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The Caii–Mv Correlation (Wilson‐Bappu Effect) Calibrated by Hipparcos Parallaxes
TL;DR: In this article, a linear relationship similar to the one derived originally by Wilson & Bappu and improved by Lutz & Kelker was found from Mv = +7 to 2.
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Spectroscopy of low surface brightness galaxies with the Hobby-Eberly Telescope
TL;DR: In this paper, low-resolution spectra of 19 red and blue low surface brightness (LSB) galaxies were obtained using the Marcario Low-Resolution Spectrograph on the 9.2 m Hobby-Eberly Telescope.
Journal ArticleDOI
Catalogue of Large Magellanic Cloud star clusters observed in the Washington photometric system
Tali Palma,Tali Palma,Tali Palma,L. V. Gramajo,Juan J. Clariá,Juan J. Clariá,Marcelo Lares,Marcelo Lares,Marcelo Lares,Doug Geisler,Andrea Veronica Ahumada,Andrea Veronica Ahumada +11 more
TL;DR: In this paper, the authors compile a catalogue including the fundamental parameters of a complete sample of 277 star clusters (SCs) of the Large Magellanic Cloud (LMC) observed in the Washington photometric system, including 82 clusters very recently studied by them.
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The origin of the supersoft X-ray--optical/UV flux anticorrelation in the symbiotic binary AG Draconis
TL;DR: In this paper, the authors identify the source of the X-ray emission and reveal the nature of the observed flux anticorrelation in the white dwarf photosphere using XMM-Newton, far-UV spectroscopy from FUSE, low-and high-resolution IUE spectra and optical/near-IR spectroscopic and/or photometric observations.