Access to Astronomical Catalogues

← Click to display the menu
J/A+A/445/69        JHK' photometry of C stars in NGC 147          (Sohn+, 2006)

Near-IR photometry of asymptotic giant branch stars in the dwarf elliptical galaxy NGC 147. Sohn Y.J., Kang A., Rhee J., Shin M., Chun M.S., Kim H.I. <Astron. Astrophys. 445, 69 (2006)> =2006A&A...445...69S
ADC_Keywords: Galaxies, nearby ; Photometry, infrared ; Stars, carbon ; Stars, giant Keywords: galaxies: individual: NGC 147 - galaxies: stellar content - stars: AGB and post-AGB Abstract: Near-infrared J, H and K' images were used to investigate the stellar contents of the asymptotic giant branch (AGB) population in the nearby dwarf elliptical galaxy NGC 147. The obtained (K,J-K) and (K,H-K) color-magnitude diagrams contain stars of AGB and red giant branch populations, where the former consists of a group of bright blue stars, a dominant population of M giant and a red C star population.We identified 91 AGB C stars in NGC 147 with the mean absolute magnitude and colors of <MK≥-7.56, <(J-K)0≥1.81 and <(H-K)0≥0.74. The estimated number ratio of C stars to M giant stars (C/M) is 0.16±0.02. The estimated local C/M ratios of 0.14±0.02 for the inner region (r<70") and 0.19±0.03 for the outer region (r>70") indicate a weak radial gradient. The mean bolometric magnitude of 91 C stars in NGC 147 is <Mbol≥-4.32±0.49. The bolometric luminosity function of M giant stars in NGC 147 extends up to Mbol=-5.8 magnitude, and that of only C stars spans -5.6<Mbol←3.5. The color histograms of AGB stars in (J-K) and (H-K) show a main peak containing M giant stars, a red tail containing C stars with a weak excess, and a blue excess possibly due to bright blue foreground stars and AGB stars younger than M giants. The comparison of the theoretical isochrone models with the color distribution and the brightness of AGB stars indicates that most of the bright M giants in NGC 147 were formed at log(tyr)∼8.4 with a range of 8.2∼8.6. Ages of the majority of M giant stars in NGC 147 are similar to those of younger M giant stars in its companion NGC 185, while their formation occurred more recently than the older M giant stars in NGC 185 by ∼2Gyrs. Description: The equatorial coordinates, near-infrared photometric properties of 91 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/418/33). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 82 91 Coordinates and near-IR photometric properties for 91 C stars
See also: J/A+A/403/93 : Photometry of AGB stars in NGC 185 and NGC 147 (Nowotny+, 2003) J/A+A/418/33 : RI photometry of C stars in NGC 147 (Battinelli+, 2004) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Seq ID number of C star 4- 5 I2 h RAh Right Ascension J2000 (hours) 7- 8 I2 min RAm Right Ascension J2000 (minutes) 10- 14 F5.2 s RAs Right Ascension J2000 (seconds) 16 A1 --- DE- Declination J2000 (sign) 17- 18 I2 deg DEd Declination J2000 (degrees) 20- 21 I2 arcmin DEm Declination J2000 (minutes) 23- 26 F4.1 arcsec DEs Declination J2000 (seconds) 28- 33 F6.3 mag K'mag K' band (2.12um) magnitude of C star 35- 39 F5.3 mag e_K'mag Error of K magnitude 41- 45 F5.3 mag (J-K') (J-K') color index 47- 51 F5.3 mag e_(J-K') Error of (J-K') color index 53- 57 F5.3 mag (H-K') (H-K') color index 59- 63 F5.3 mag e_(H-K') Error of (H-K') color index 65- 68 F4.2 mag (V-i)0 ? (V-i) color index by Nowotny et al., 2003, Cat. J/A+A/403/93 70- 72 I3 --- Nowotny ? ID number of Nowotny et al., 2003, Cat. J/A+A/403/93, recno number in Vizir 74- 78 F5.3 mag R-I ? (R-I) color index by Battinelli & Demers, 2004, Cat. J/A+A/418/33 80- 82 I3 --- [BD2004c] ? ID number of Battinelli & Demers, 2004, Cat. J/A+A/418/33
Acknowledgements: Aram Kang, breeze82(at)galaxy.yonsei.ac.kr
(End) Patricia Vannier [CDS] 06-Sep-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

catalogue service

© UDS/CNRS

Contact