T Tauri in and around bright-rimmed clouds

The aim of this paper is to quantitatively testify the 'small-scale sequential star formation' hypothesis in and around bright-rimmed clouds (BRCs). As a continuation of the recent attempt by Ogura et al. (2007PASJ...59..199O), we have carried out BVIc photometry of four more BRC aggregates along with deeper re-observations of two previously observed BRCs. Again, quantitative age gradients are found in almost all the BRCs studied in the present work. Archival Spitzer/Infrared Array Camera data also support this result.

Cone search capability for table J/MNRAS/396/964/stars (Optical and near-IR photometry and physical)

Cone search capability for table J/MNRAS/396/964/table6 (IRAC photometric magnitudes of the disk bearing candidates in BRCs 2, 27 and 13/14)

Cone search capability for table J/MNRAS/396/964/table7 (J, H and K magnitudes of the sources used in the analysis (cf. Sect. 6.2))

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/396/964
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/396/964
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/396/964
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/396/964
Provenance
Creator Chauhan N.; Pandey A.K.; Ogura K.; Ojha D.K.; Bhatt B.C.; Ghosh S.K.; Rawat P.S.
Publisher CDS
Publication Year 2010
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; Stellar Astronomy