Multiwavelength study of NGC 7419 : J/MNRAS/391/1279

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Authors : Joshi H. orcid , Kumar B., Singh K.P. (hide) , Kumar B., Singh K.P. et..al

VizieR DOI : 10.26093/cds/vizier.73911279
Bibcode : 2008MNRAS.391.1279J (ADS) (Simbad) (Objects)
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CDS Keywords : Clusters, open; Photometry, UBVRI; Photometry, H-alpha; X-ray sources
UAT : Open star clusters, Infrared photometry, Optical astronomy, Broad band photometry, Optical astronomy, H alpha photometry, X-ray sources

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Inserted into VizieR : 10-Jun-2009
Last modification : 07-Jul-2024

Multiwavelength study of a young open cluster NGC7419. (2008)

Keywords : stars emission-line, Be - stars: formation - stars: pre-main-sequence - X-rays: galaxies: clusters - X-rays: stars

Abstract:Using new UBVRI H{alpha} CCD photometric observations and the archival infrared and X-ray data, we have carried out a multiwavelength study of a Perseus arm young open star cluster NGC 7419. Using XMM-Newton observations, we found several X-ray sources in the cluster region but none of the Herbig Ae/Be stars is detected in X-rays. ...(more)
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The optical observations of NGC 7419 were carried out using a thinned back-illuminated CCD camera mounted at f/13 Cassegrain focus of the 104-cm Sampurnanand reflector telescope of Aryabhatta Research Institute of Observational Sciences, Nainital. Broad-band Johnson UBV, Cousins RI and narrow-band H{alpha} line ({lambda}=656.5nm) and H{alpha} continuum ({lambda}=665nm) filters were used for observations. 


                


                

                    

                


                

                    

                


                

                    
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