Interstellar reddening in 3 HII regions

The slope of the interstellar reddening line in the J-H vs. H-Ks diagram of the 2MASS survey in the direction of the North America and Pelican nebulae, the L 935 dust cloud and the Cyg OB2 association is determined. The MK types were either classified by C.J. Corbally or collected from the literature. The ratio E(J-H)/E(H-Ks)=2.0 is obtained by taking the average for the four groups of spectral classes: O3-B1, B2-B6, B7-B9.5 and red clump giants. The obtained ratio is among the largest values of E(J-H)/E(H-Ks) determined till now.

Cone search capability for table J/BaltA/17/125/table1 (O-B stars in the vicinity of the North America and Pelican nebulae and in the Cyg OB2 association)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/BaltA/17/125
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/BaltA/17/125
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/BaltA/17/125
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/BaltA/17/125
Provenance
Creator Straizys V.; Corbally C.J.; Laugalys V.
Publisher CDS
Publication Year 2008
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; Interstellar medium; Natural Sciences; Observational Astronomy; Physics