J/MNRAS/443/454     UBVIHα photometry in NGC 1893            (Lim+, 2014)

Sejong Open Cluster Survey (SOS). III. The young open cluster NGC 1893 in the HII region W8. Lim B., Sung H., Kim J.S., Bessell M.S., Park B.-G. <Mon. Not. R. Astron. Soc., 443, 454-473 (2014)> =2014MNRAS.443..454L 2014MNRAS.443..454L
ADC_Keywords: Clusters, open ; Photometry, UBVRI ; Photometry, H-alpha Keywords: accretion, accretion discs - circumstellar matter - stars: luminosity function, mass function - open clusters and associations: individual: NGC 1893 Abstract: We present a UBVI and Hα photometric study of the young open cluster NGC 1893 in the HII region W8 (IC 410 or Sh 2-236). A total of 65 early-type members are selected from photometric diagrams. A mean reddening of the stars is <E(B-V)≥0.563±0.083mag. The published photometric data in the near- and mid-infrared passbands are used to test the reddening law towards the cluster, and we confirm that the reddening law is normal (RV=3.1). Zero-age main-sequence fitting gives a distance modulus of V0-MV= 12.7±0.2mag, equivalent to 3.5±0.3kpc. From Hα photometry, 125 Hα emission stars and candidates are identified as pre-main-sequence (PMS). The lists of young stellar objects and X-ray sources published by previous studies allow us to select a large number of PMS members down to 1M. Isochrone fitting in the Hertzsprung-Russell diagram gives a turn-off age of 1.5Myr and the median age of 1.9Myr from the PMS members with a spread of ∼5Myr. We derive the initial mass function (IMF) for stars with mass larger than 1M. The slope of the IMF (Γ=-1.3±0.1) is well consistent with the Salpeter/Kroupa IMF. A total mass of the cluster appears to be in excess of 1300M. Finally, we estimate the mass accretion rate of 82 PMS members in the mass range of 0.6-5M. Description: The observation of NGC 1893 was made on 2009 January 19 using the AZT-22 1.5m telescope (f/7.74) at Maidanak Astronomical Observatory in Uzbekistan. All imaging data were acquired using the Fairchild 486 CCD (SNUCam) with the standard Bessell UBVI and Hα filters. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 152 6503 Photometric data -------------------------------------------------------------------------------- See also: J/MNRAS/438/1451 : UBVIHa photometry of IC 1848 (Lim+, 2014) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID [-18/6485] Sequential number (1) 6- 7 I2 h RAh Right ascension (J2000) 9- 10 I2 min RAm Right ascension (J2000) 12- 16 F5.2 s RAs Right ascension (J2000) 18 A1 --- DE- Declination sign (J2000) 19- 20 I2 deg DEd Declination (J2000) 22- 23 I2 arcmin DEm Declination (J2000) 25- 28 F4.1 arcsec DEs Declination (J2000) 30- 35 F6.3 mag Vmag [9/23.2]? Bessel V magnitude 37- 42 F6.3 mag Imag [10.3/21.3]? Bessel I magnitude 44- 48 F5.3 mag V-I ? V-I colour index 50- 55 F6.3 mag B-V ? B-V colour index 57- 62 F6.3 mag U-B ? U-B colour index 64- 69 F6.3 mag H-C ? Hα index (C=(V+I)/2) 71- 76 F6.3 mag e_Vmag ? rms uncertainty on Vmag 78- 82 F5.3 mag e_Imag ? rms uncertainty on Imag 84- 88 F5.3 mag e_V-I ? rms uncertainty on V-I 90- 94 F5.3 mag e_B-V ? rms uncertainty on B-V 96-100 F5.3 mag e_U-B ? rms uncertainty on U-B 102-106 F5.3 mag e_H-C ? rms uncertainty on H-C 108 I1 --- o_Vmag [0/2] Number of observations for Vmag 110 I1 --- o_Imag [0/2] Number of observations for Imag 112 I1 --- o_V-I [0/2] Number of observations for V-I 114 I1 --- o_B-V [0/2] Number of observations for B-V 116 I1 --- o_U-B [0/2] Number of observations for U-B 118 I1 --- o_H-C [0/2] Number of observations for H-C 120-135 A16 --- 2MASS 2MASS name (HHMMSSss+DDMMSSs) 137 A1 --- em [Hh] Hα emission flag (2) 139-152 A14 --- SpType Spectral type for stars -1 to -18 (3) -------------------------------------------------------------------------------- Note (1): The negative numbered ID represents the data from Johnson & Morgan (1955ApJ...122..142J 1955ApJ...122..142J); Hiltner (1956ApJS....2..389H 1956ApJS....2..389H); Hoag et al. (1961PUSNO..17..343H 1961PUSNO..17..343H); Cuffey (1973AJ.....78..408C 1973AJ.....78..408C); Massey et al. (1995ApJ...454..151M 1995ApJ...454..151M, Cat. J/ApJ/454/151); Hog et al. (2000A&A...355L..27H 2000A&A...355L..27H, Cat. I/259) Note (2): Halpha flag as follows: H = Hα emission stars h = Hα emission star candidates Note (3): Spectral type for stars -1 to -12, from Hoag & Applequist (1965ApJS...12..215H 1965ApJS...12..215H); Massey et al. (1995ApJ...454..151M 1995ApJ...454..151M, Cat. J/ApJ/454/151); Negueruela et al. (2007A&A...471..485N 2007A&A...471..485N); Sota et al. (2011ApJS..193...24S 2011ApJS..193...24S, Cat. III/274) -------------------------------------------------------------------------------- History: From electronic version of the journal References: Sung et al., 2013JKAS...46..103S 2013JKAS...46..103S Lim et al., Paper II 2014MNRAS.438.1451L 2014MNRAS.438.1451L, Cat. J/MNRAS/438/1451
(End) Patricia Vannier [CDS] 10-Mar-2015
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