J/A+A/330/990    VRIJHK photometry of the Serpens cloud core (Giovannetti+ 1998)

Deep optical and near infrared imaging photometry of the Serpens cloud core Giovannetti P., Caux E., Nadeau D., Monin J.-L. <Astron. Astrophys. 330, 990 (1998)> =1998A&A...330..990G 1998A&A...330..990G (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, open ; Stars, pre-main sequence ; Photometry, infrared Keywords: stars: pre-main sequence - ISM: open clusters: Serpens cloud - stars: luminosity function - infrared: stars - star formation Abstract: We present results from a deep optical (VRI) and near infrared (JHK) survey of the central part of the Serpens molecular cloud. A total of 138 sources were detected in the 19 arcmin2 surveyed area down to a limiting magnitude of 16.3 in K. We find that the form of the observed K Luminosity Function (KLF) of stars belonging to the Serpens Molecular cloud is consistent with that predicted from a Miller & Scalo (1979ApJS...41..513M 1979ApJS...41..513M) Interstellar Mass Function (IMF). We have investigated the KLF evolution with the age of a cluster by modeling KLFs of hypothetical clusters. Our results suggest that two phases of star formation could have taken place in the Serpens core. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2 109 165 Log of observations table2.tex 123 219 Latex version of table2 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Name Sequential object number 4 A1 --- n_Name [S] S: Serpens cloud members 6- 7 I2 h RAh Right ascension (1950) 9- 10 I2 min RAm Right ascension (1950) 12- 15 F4.1 s RAs Right ascension (1950) 16 A1 --- DE- Declination sign 17- 18 I2 deg DEd Declination (1950) 20- 21 I2 arcmin DEm Declination (1950) 23- 24 I2 arcsec DEs Declination (1950) 26- 27 A2 --- n_Vmag Note on Vmag (1) 29- 32 F4.1 mag Vmag ? V magnitude 34- 37 F4.2 mag e_Vmag ? 3 σ uncertainty on Vmag 39- 40 A2 --- n_Rmag Note on Rmag (1) 42- 45 F4.1 mag Rmag ? R magnitude 47- 50 F4.2 mag e_Rmag ? 3 σ uncertainty on Rmag 52- 53 A2 --- n_Imag Note on Imag (1) 55- 58 F4.1 mag Imag ? I magnitude 60- 63 F4.2 mag e_Imag ? 3 σ uncertainty on Imag 65- 66 A2 --- n_Jmag Note on Jmag (1) 68- 71 F4.1 mag Jmag ? J magnitude 73- 76 F4.2 mag e_Jmag ? 3 σ uncertainty on Jmag 78- 79 A2 --- n_Hmag Note on Hmag (1) 81- 84 F4.1 mag Hmag ? H magnitude 86- 89 F4.2 mag e_Hmag ? 3 σ uncertainty on Hmag 91- 92 A2 --- n_Kmag Note on Kmag (1) 94- 97 F4.1 mag Kmag ? K magnitude 99-102 F4.2 mag e_Kmag ? 3 σ uncertainty on Kmag 104-109 A6 --- Other Other identification (2) -------------------------------------------------------------------------------- Note (1): x: Regions of the sky that were not observed in the concerned photometric band nd: Sources that were not detected Note (2): CK: Churchwell and Koornneef (1986ApJ...300..729C 1986ApJ...300..729C) EC: Eiroa and Casali (1992A&A...262..468E 1992A&A...262..468E) GEL: Gomez de Castro et al. (1988A&A...201..299G 1988A&A...201..299G) HCE: Horrobin et al. (1997A&A...320L..41H 1997A&A...320L..41H) -------------------------------------------------------------------------------- Acknowledgements: Philippe Giovannetti
(End) Patricia Bauer [CDS] 04-Sep-1997
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