A review of the distance and structure of the Large Magellanic Cloud
- 1 July 2004
- journal article
- review article
- Published by Elsevier in New Astronomy Reviews
- Vol. 48 (9) , 659-665
- https://doi.org/10.1016/j.newar.2004.03.001
Abstract
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This publication has 33 references indexed in Scilit:
- The MACHO Project Large Magellanic Cloud Variable-Star Inventory. XIII. Fourier Parameters for the First-Overtone RR Lyrae Variables and the LMC DistanceThe Astronomical Journal, 2004
- Eclipsing binaries in the Magellanic CloudsAstronomy & Astrophysics, 2003
- Distance to the Large Magellanic Cloud: The RR Lyrae StarsThe Astronomical Journal, 2003
- Astrometry with the [ITAL]Hubble Space Telescope[/ITAL]: A Parallax of the Fundamental Distance Calibrator δ CepheiThe Astronomical Journal, 2002
- On the Distance of Magellanic Clouds: First Overtone CepheidsThe Astrophysical Journal, 2002
- [ITAL]K[/ITAL]-Band Red Clump Distance to the Large Magellanic CloudThe Astrophysical Journal, 2002
- Theoretical Models for Bump CepheidsThe Astrophysical Journal, 2002
- Astrometry with the [ITAL]Hubble Space Telescope[/ITAL]: A Parallax of the Fundamental Distance Calibrator RR LyraeThe Astronomical Journal, 2002
- A Step toward the Calibration of the Red Giant Branch Tip as a Standard CandleThe Astrophysical Journal, 2001
- The Rotation Curve of the Large Magellanic Cloud and the Implications for MicrolensingThe Astrophysical Journal, 2000