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J/AJ/122/866        X-ray sources in IC 348 from Chandra     (Preibisch+, 2001)

Deep Chandra X-ray observatory imaging study of the very young stellar cluster IC 348. Preibisch T., Zinnecker H. <Astron. J. 122, 866 (2001)> =2001AJ....122..866P
ADC_Keywords: Clusters, open ; X-ray sources Mission_Name: Chandra Keywords: open clusters and associations: individual (IC 348) - stars: coronae - stars: low-mass, brown dwarfs - stars: pre-main-sequence - X-rays Abstract: We have obtained a deep (53 ks) X-ray image of the very young stellar cluster IC 348 with the Advanced CCD Imaging Spectrometer on board the Chandra X-Ray Observatory. In our image with a sensitivity limit of ∼1x1028ergs/s (more than 10 times deeper than our ROSAT images of IC 348), 215 X-ray sources are detected. While 115 of these sources can be identified with known cluster members, 58 X-ray sources are most likely new, still unidentified cluster members. About 80% of all known cluster members with masses between ∼0.15 and 2M are visible as X-ray sources in our image. We discover X-ray emission at levels of ∼1028ergs/s from four of 13 known brown dwarfs and from three of 12 brown dwarf candidates in IC 348. We also detect X-ray emission from two deeply embedded objects, presumably class I protostars, south of the cluster center. Description: File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 51 215 ACIS X-ray Sources in IC 348 table2.dat 104 25 Brown dwarfs and brown dwarfs candidates in IC 348
See also: J/A+A/324/549 : Deep UVBRI photometry in IC 348 (Trullols+ 1997) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- CXOPZ Source number 6 I1 h RAh Right Ascension (J2000) 8- 9 I2 min RAm Right Ascension (J2000) 11- 15 F5.2 s RAs Right Ascension (J2000) 17 A1 --- DE- Declination sign (J2000) 18- 19 I2 deg DEd Declination (J2000) 21- 22 I2 arcmin DEm Declination (J2000) 24- 27 F4.1 arcsec DEs Declination (J2000) 30- 33 F4.1 arcsec e_RAs Right Ascension position uncertainty 35- 38 F4.1 arcsec e_DEs Declination position uncertainty 41- 45 F5.2 ct/ks CR Count rate 48- 51 F4.2 ct/ks e_CR Error in CR
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 3 A3 --- Origin L99: Objects from Luhman, 1999ApJ...525..466L N00: Additional objects from Najita et al., 2000ApJ...541..977N 5- 10 A6 --- Object Object identification (1) 12- 17 A6 --- SpType Spectral type 18- 20 F3.1 --- e_SpType ? Uncertainty on sub-type 22- 24 A3 --- Class Classification (2) 27- 31 F5.2 mag AVmag Absorption in V band 32 A1 --- u_AVmag Uncertainty flag on AVmag 34- 39 F6.4 solLum Lbol Bolometric luminosity 41- 42 A2 --- l_Massl [~< ] Limit flag on Massl 43- 46 F4.2 solMass Massl Mass, lower limit (3) 49- 52 F4.2 solMass Massu ? Mass, upper limit (3) 54 A1 --- l_ACIS Limit flag on ACIS 55- 58 F4.1 ct ACIS Number of background-subtracted source counts detected in the ACIS image 60- 62 F3.1 --- e_ACIS ? rms uncertainty on ACIS 64 A1 --- l_Lx Limit flag on Lx 65- 68 F4.1 10+21W Lx X-ray luminosity (4) 70- 72 F3.1 10+21W e_Lx ? rms uncertainty on Lx 74 A1 --- l_log(Lx/Lbol) Limit flag on log(Lx/Lbol) 75- 78 F4.1 --- log(Lx/Lbol) X-ray to bolometric luminosity ratio 81- 82 I2 h RAh Right ascension (J2000) 84- 85 I2 min RAm Right ascension (J2000) 87- 91 F5.2 s RAs Right ascension (J2000) 93 A1 --- DE- Declination sign (J2000) 94- 95 I2 deg DEd Declination (J2000) 97- 98 I2 arcmin DEm Declination (J2000) 100-103 F4.1 arcsec DEs Declination (J2000)
Note (1): Luhman 1999: Cl* IC 348 LRL NNN in Simbad Note (2): (BD) brown dwarf; (BDC) brown dwarf candidate. Note (3): Range of the mass estimates given by the different models and temperature scales. Note (4): Dereddened 0.2-8 keV-band X-ray luminosity based on the exposure time-corrected source count rate computed assuming a Raymond-Smith plasma spectrum with kT=1keV.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 10-Sep-2001
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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