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J/A+A/437/61        Near-IR photometry of AGB stars in NGC 185    (Kang+, 2005)

Near-IR photometry of asymptotic giant branch stars in the dwarf elliptical galaxy NGC 185. Kang A., Sohn Y.-J., Rhee J., Shin M., Chun M.-S., Kim H.-I. <Astron. Astrophys. 437, 61 (2005)> =2005A&A...437...61K
ADC_Keywords: Stars, giant ; Stars, carbon ; Photometry, infrared Keywords: galaxies: individual: NGC 185 - galaxies: stellar content - stars: AGB and post-AGB Abstract: J, H and K' images obtained with the Canada-France-Hawaii Telescope were used to investigate the stellar contents of asymptotic giant branch (AGB) in the dwarf elliptical galaxy NGC 185. The bright parts of (K, J-K) and (K, H-K) color-magnitude diagrams consist of a group of brights blue stars, a dominant populations of M-giants, and a red C star population. There were 73 C stars with a mean magnitude of <K≥16.26±0.38, corresponding to <MK≥-7.93 and mean colors of <(J-k)0≥2.253 and <(H-K)0≥0.865. The number ratio of C stars to M-giants was estimated to be 0.11±0.04 without any radial gradient from the center of NGC 185. The (J-K) and (H-K) color distributions of AGB stars showed an M-giant pick, blue and red tails, where the latter two correspond to AGB stars younger than those along M-giant peak and C stars. The bolometric luminosity functions of M-giants and C stars indicated that the M-giant AGB sequence has terminated at Mbol=-6.2, while the most luminous C star very similar to that of Nowotny et al. (2003, Cat. J/A+A/403/93) which was derived from VI band photometry. The logarithmic slope of the luminosity function for bright M-giant stars was estimated to be 0.83±0.02 in K band. Theoritical isochrone models, compared with the observed near-infrared photometric properties of AGB stars, indicated that the star formation in NGC 185 has a wide range of age span with possibly two different epochs of star formation. Description: Table2 contains the equatorial coordinates, near-infrared photometric properties of 73 C stars, and color indices in VRI bands of cross-identified C stars with Nowotny et al. (2003, Cat. J/A+A/403/93) and Battinelli & Demers (2004, Cat. J/A+A/417/479). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 98 73 Coordinates and near-IR photometric properties for 73 C stars
See also: J/A+A/417/479 : RI photometry of NGC 185 carbon stars (Battinelli+, 2004) J/A+A/403/93 : Photometry of AGB stars in NGC 185 and NGC 147 (Nowotny+, 2003) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Seq Identification number of C star 6- 7 I2 h RAh Right Ascension J2000 (hours) 9- 10 I2 min RAm Right Ascension J2000 (minutes) 12- 16 F5.2 s RAs Right Ascension J2000 (seconds) 18 A1 --- DE- Declination J2000 (sign) 19- 20 I2 deg DEd Declination J2000 (degrees) 22- 23 I2 arcmin DEm Declination J2000 (minutes) 25- 28 F4.1 arcsec DEs Declination J2000 (seconds) 31- 36 F6.3 mag Jmag J band magnitude of C star 38- 42 F5.3 mag e_Jmag Error of J magnitude 45- 49 F5.3 mag (J-K) (J-K) colour index 51- 55 F5.3 mag e_(J-K) Error of (J-K) colour 58- 62 F5.3 mag (H-K) (H-K) colour index 64- 68 F5.3 mag e_(H-K) Error of (H-K) colour 71- 74 F4.2 mag (V-i)o ? (V-i) colour by Nowotny et al. (2003, Cat. J/A+A/403/93) 76- 78 I3 --- Nint ? Internal number for [NKO2003] source 80- 87 I8 --- [NKO2003] ? Identification number of Nowotny et al. (2003, Cat. J/A+A/403/93), [NKO2003] NGC 185 NNNNNNNN in Simbad 90- 94 F5.3 mag R-I ? (R-I) color by Battinelli & Demers (2004, Cat. J/A+A/417/479) 96- 98 I3 --- [BD2004b] ? Identification number of Battinelli & Demers (2004, Cat. J/A+A/417/479)
Acknowledgements: Aram Kang, breeze82(at)galaxy.yonsei.ac.kr
(End) Patricia Vannier [CDS] 21-Mar-2005
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

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