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The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. IV. Long-Period Variables in the Large Magellanic Cloud

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arxiv 0910.1354 v1 pith:4Q237A3O submitted 2009-10-07 astro-ph.SR

classification astro-ph.SR
keywords starssrvscatalogvariablescloudlargelong-periodlpvs
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The fourth part of the OGLE-III Catalog of Variable Stars presents 91 995 long-period variables (LPVs) in the Large Magellanic Cloud (LMC). This sample consists of 79 200 OGLE Small Amplitude Red Giants (OSARGs), 11 128 semiregular variables (SRVs) and 1667 Mira stars. The catalog data include basic photometric and astrometric properties of these stars, long-term multi-epoch VI photometry and finding charts. We describe the methods used for the identification and classification of LPVs. The distribution of I-band amplitudes for carbon-rich stars shows two maxima, corresponding to Miras and SRVs. Such a distinction between Miras and SRVs is not obvious for oxygen-rich stars. We notice additional period-luminosity sequence located between Wood's sequences C and C' and populated by SRVs.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 5 citations worldwide. Full citation record

  1. The Carbon Giant Population Revealed by Gaia DR3

    astro-ph.SR 2026-08 conditional novelty 6.0 of 10

    A uniform Gaia DR3 census of carbon giants separates intrinsic AGB stars from extrinsic post-mass-transfer giants and measures their space densities, scale heights, and radial distribution in the Milky Way.

  2. eRASSU J043115.8-711730 :the first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    J0431-71 is a new super-soft X-ray symbiotic binary in the Magellanic Bridge whose ~524-day optical pulsation appears to drive variable accretion onto a white dwarf.

  3. Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant

    astro-ph.GA 2019-08 conditional novelty 6.0 of 10

    A corrected LMC TRGB calibration on the HST photometric system yields M_F814W = -3.97 +/- 0.046 mag and raises the TRGB-based Hubble constant from 69.8 to 72.4 +/- 2.0 km/s/Mpc.

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