LMC type II Cepheids JHKs magnitudes

DOI

JHKs magnitudes corrected to mean intensity are estimated for Large Magellanic Cloud (LMC) type II Cepheids in the OGLE-III survey the third phase of the Optical Gravitational Lensing Experiment (OGLE). Period-luminosity (PL) relations are derived in JHKs as well as in a reddening-free VI parameter. Within the uncertainties, the BL Her stars (P<4d) and the W Vir stars (P=4 to 20d) are colinear in these PL relations. The slopes of the infrared relations agree with those found previously for type II Cepheids in globular clusters within the uncertainties.

Cone search capability for table J/MNRAS/397/933/table2 (The catalogue of S08 (Soszynski et al., Cat. J/AcA/58/293) sources with IRSF counterparts)

Identifier
DOI http://doi.org/10.26093/cds/vizier.73970933
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/397/933
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/397/933
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/397/933
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/397/933
Provenance
Creator Matsunaga N.; Feast M.W.; Menzies J.W.
Publisher CDS
Publication Year 2012
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy