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J/ApJ/641/410    XMM and Chandra X-ray sources near 4U 1755-33   (Kaaret+, 2006)

Evolution of the X-ray jets from 4U 1755-33. Kaaret P., Corbel S., Tomsick J.A., Lazendic J., Tzioumis A.K., Butt Y., Wijnands R. <Astrophys. J., 641, 410-417 (2006)> =2006ApJ...641..410K
ADC_Keywords: X-ray sources ; Binaries, X-ray Keywords: black hole physics - stars: individual (4U 1755-33) - stars: winds, outflows - X-rays: binaries Abstract: We report on new X-ray observations of the large-scale jets recently discovered in X-rays from the black hole candidate 4U 1755-33. Our observations in 2004 show that the jets found in 2001 are still present in X-rays. However, sensitive radio observations in 2004 failed to detect the jets. Description: We observed 4U 1755-33 using XMM-Newton beginning on 2004 September 18 (observation B). We also analyzed an archival observation obtained by Angelini & White (2003ApJ...586L..71A) beginning on 2001 March 8 (observation A). On 2004 April 27, we obtained continuum radio observations of 4U 1755-33 using the Australia Telescope Compact Array (ATCA) located in Narrabri, New South Wales, Australia. To determine if the features found in the XMM-Newton X-ray image are point sources or truly diffuse emission, we analyzed two Chandra observations obtained of the same field, on 2003 September 25 and on 2004 June 25. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 82 27 XMM-Newton X-ray sources near 4U 1755-33 table3.dat 82 56 Chandra X-ray sources near 4U 1755-33
Byte-by-byte Description of file: table1.dat table3.dat
Bytes Format Units Label Explanations
1- 2 I2 --- [KCT2006] Source number (1) 4- 5 I2 h RAh Hour of Right Ascension (J2000) 7- 8 I2 min RAm Minute of Right Ascension (J2000) 10- 15 F6.3 s RAs Second of Right Ascension (J2000) 17 A1 --- DE- Sign of the Declination (J2000) 18- 19 I2 deg DEd Degree of Declination (J2000) 21- 22 I2 arcmin DEm Arcminute of Declination (J2000) 24- 28 F5.2 arcsec DEs Arcsecond of Declination (J2000) 30- 32 F3.1 arcsec ePos Statistical source position error (2) 34 A1 --- n_Flux1 [A3] Indicates the date of observation of the first flux (3) 36- 40 F5.1 10-17W/m2 Flux1 ? First 0.3-10keV flux (4) 42- 45 F4.1 10-17W/m2 e_Flux1 ? Uncertainty in Flux1 47 A1 --- n_Flux2 [B4] Indicates the date of observation of the second flux (3) 49- 53 F5.1 10-17W/m2 Flux2 ? Second 0.3-10keV flux (4) 55- 58 F4.1 10-17W/m2 e_Flux2 ? Uncertainty in Flux2 60- 76 A17 --- xID Counterpart (5) 78- 82 A5 --- 2MASS [2mass] 2MASS counterpart (Cat. II/246)
Note (1): Source number is: Table 1: [KCT2006] XMM NN in Simbad Table 3: [KCT2006] Chandra NN in Simbad Note (2): This does not include errors in the overall astrometry. Note (3): The date of observation are coded as follows: A = refers to an XMM-Newton archival observation obtained by Angelini & White (2003ApJ...586L..71A) beginning on 2001-Mar-08 with a duration of 19.4ks (ObsID 0032940101) (Table 1 only) B = refers to an XMM-Newton observation beginning on 2004-Sep-18 for 45.9ks (ObsID 0203750101) (Table 1 only) 3 = refers to a 22ks exposure Chandra observation obtained on 2003-Sep-25 (ObsID 3510; PI S. Murray) (Table 3 only) 4 = refers to a 45ks exposure Chandra observation obtained on 2004-Jun-25 (ObsID 4586; PI L. Angelini) (Table 3 only) Note (4): In units of 10-14erg/cm2/s and calculated assuming a power law spectrum with photon index of 1.5 and corrected for the Galactic absorption column density of 3.1x1021cm-2. Note (5): Counterparts in Angelini & White (2003ApJ...586L..71A, [AW2003] N in Simbad), or the XMM sources in Table 1 (XMM NN).
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 04-Apr-2008
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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