J/other/NewA/17.160   UBVRI photometry of Stock 18           (Bhatt+, 2012)

Stellar contents and star formation in the young cluster Stock 18. Bhatt H., Sagar R., Pandey J.-C. <New Astron., 17, 160-166 (2012)> =2012NewA...17..160B 2012NewA...17..160B
ADC_Keywords: Clusters, open ; Photometry, UBVRI ; Photometry, CCD Keywords: young cluster - star formation - mass function - mass segregation individual: Stock 18 Abstract: We have carried out deep (V∼21mag) UBVRI photometric study of the star cluster Stock 18. These along with archival Infrared data have been used to derive the basic cluster parameters and also to derive the basic cluster parameters and also to study the star for formation processes in and around the cluster region. The distance to the cluster is derived as 2.8±0.2kpc while its age is estimated as 6.0±2.0Myr. Present study indicates that interstellar reddening is normal in the direction of the cluster. The mass function slope is found to be -1.37±0.27 for the mass range 1<M/M<11.9. There is no evidence found for the effect of mass segregation in main-sequence stars of the cluster. A young stellar population with age between 1-2Myr have been found in and around the cluster region. The presence of IRAS and AKARI sources with MSX intensity map also show the youth of the Sh2-170 region. Description: The CCD UBVRI photometric data were acquired using 104-cm Sampurnanand Telescope (ST) of ARIES, Nainital, on 08/10/2007 and 19/12/2006. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 88 2261 *UBVRI photometric data of the sample stars in 13'x13' region -------------------------------------------------------------------------------- Note on table2.dat: CCD positions of stars are converted into RAJ2000 and DECJ2000 using the Guide Star Catalogue II (GSC 2.2, 2001). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- Seq [1/2261] Sequential number 6- 13 F8.6 deg RAdeg Right ascension in decimal degrees (J2000) 15- 23 F9.6 deg DEdeg Declination in decimal degrees (J2000) 25- 30 F6.3 mag Umag ?=- Landolt U magnitude 32- 36 F5.3 mag e_Umag ?=- rms uncertainty on Umag 38- 43 F6.3 mag Bmag ?=- Landolt B magnitude 45- 49 F5.3 mag e_Bmag ?=- rms uncertainty on Bmag 51- 56 F6.3 mag Vmag ?=- Landolt V magnitude 58- 62 F5.3 mag e_Vmag ?=- rms uncertainty on Vmag 64- 69 F6.3 mag Rmag ?=- Landolt R magnitude 71- 75 F5.3 mag e_Rmag ?=- rms uncertainty on Rmag 77- 82 F6.3 mag Imag ?=- Landolt I magnitude 84- 88 F5.3 mag e_Imag ?=- rms uncertainty on Umag -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 23-Mar-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line