J/A+A/430/287       XMM observations of IC 2391 stars        (Marino+, 2005)

X-ray spectral and timing characteristics of the stars in the young open cluster IC 2391. Marino A., Micela G., Peres G., Pillitteri I., Sciortino S. <Astron. Astrophys., 430, 287-301 (2005)> =2005A&A...430..287M 2005A&A...430..287M
ADC_Keywords: Clusters, open ; X-ray sources ; Photometry Keywords: X-ray: stars - stars: coronae - stars: activity - stars: early-type - stars: late-type - Galaxy: open clusters and associations: individual: IC 2391 Abstract: We present X-ray spectral and timing analysis of members of the young open cluster IC 2391 observed with the XMM-Newton observatory. We detected 99 X-ray sources by analysing the summed data obtained from MOS1, MOS2 and pn detectors of the EPIC camera; 24 of them are members, or probable members, of the cluster. Stars of all spectral types have been detected, from the early-types to the late-M dwarfs. Description: We present the analysis of the Guaranteed Time XMM-Newton/EPIC observation pointed on the young open cluster IC 2391. The observation (Obs. No. 0112420101), centered on (RA=8:42:00, DE=-53:00:36), was performed on Nov. 20, 2001 during orbit 357 of XMM-Newton. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 79 99 XMM-Newton sources in the IC 2391 region, as detected in the combined EPIC image. table2.dat 87 42 X-ray and optical properties of IC 2391 members, and upper limits in the combined EPIC image. -------------------------------------------------------------------------------- See also: B/xmm : XMM-Newton Observation Log (XMM-Newton SOC, 2002) IX/37 : XMM-Newton Serendipitous Source Catalogue (1XMM) (XMM-SSC, 2003) J/MNRAS/355/959 : Proper motions of IC 2391 possible members (Dodd+, 2004) J/ApJS/134/103 : Low-mass members of IC 2391 (Barrado y Navascues+, 2001) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- [MMP2005] Sequential number 4- 13 A10 --- VRX/CTIO VRX number or (CTIO) number (1) 16- 17 I2 h RAh Right ascension (J2000.0) 19- 20 I2 min RAm Right ascension (J2000.0) 22- 27 F6.3 s RAs Right ascension (J2000.0) 29 A1 --- DE- Declination sign (J2000.0) 30- 31 I2 deg DEd Declination (J2000.0) 33- 34 I2 arcmin DEm Declination (J2000.0) 36- 40 F5.2 arcsec DEs Declination (J2000.0) 42- 47 F6.2 ks Exp Exposure time (2) 50- 55 F6.2 ct/ks CR Count Rate (2) 57- 61 F5.2 ct/ks e_CR rms uncertainty on CR (2) 63- 68 F6.2 --- Signi Probability level for the source to be a background fluctuation expressed in terms of a Gaussian-σ-equivalent. 70- 74 F5.2 --- HR ? Hardness ratio, (H-S)/(H+S) (3) 76- 79 F4.2 --- e_HR ? rms uncertainty on HR -------------------------------------------------------------------------------- Note (1): VXR, Patten & Simon, 1996ApJS..106..489P 1996ApJS..106..489P, VXR PSPC NN in Simbad. CTIO, Barrado y Navascues et al., 1999ApJ...522L..53B 1999ApJ...522L..53B and 2001ApJS..134..103B 2001ApJS..134..103B, Cl* IC 2391 CTIO NNN in Simbad. Note (2): Exposure time and X-ray count rates are expressed in "MOS1 equivalent" units. Note (3): Hardness ratio, (H-S)/(H+S), where H and S are the counts in the hard (0.8-3.5keV) and soft (0.3-0.8keV) bands, respectively. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Name (1) 9 A1 --- n_Name [ab] Note on Name (2) 11- 12 A2 --- Flag [?* #] Flag (3) 14- 15 I2 --- [MMP2005] ? Source number 17- 18 I2 h RAh Right ascension (J2000.0) 20- 21 I2 min RAm Right ascension (J2000.0) 23- 28 F6.3 s RAs Right ascension (J2000.0) 30 A1 --- DE- Declination sign (J2000.0) 31- 32 I2 deg DEd Declination (J2000.0) 34- 35 I2 arcmin DEm Declination (J2000.0) 37- 41 F5.2 arcsec DEs Declination (J2000.0) 43- 47 F5.2 mag Vmag V or I magnitude 48 A1 --- n_Vmag [I] I: I magnitude in Vmag 50- 54 F5.2 mag B-V ? B-V colour index 56- 59 F4.2 mag R-I ? R-I colour index 61- 64 F4.2 mag V-I ? V-I colour index 66 A1 --- l_CR Limit flag on CR 67- 72 F6.2 ct/ks CR Count rate 74- 75 A2 --- l_K-S [< >=] Limit flag on K-S 76- 77 I2 % K-S ? Kolmogorov-Smirnov test results (4) 78 A1 --- --- [-] 79- 80 I2 --- K-Su ? Upper limit of K-S interval (4) 82 A1 --- l_logLX Limit flag on logLX 83- 87 F5.2 [10-7W] logLX X-ray luminosity -------------------------------------------------------------------------------- Note (1): Names are from: VXR : Patten & Simon, 1996ApJS..106..489P 1996ApJS..106..489P, VXR PSPC NN in Simbad. CTIO : Barrado y Navascues et al., 1999ApJ...522L..53B 1999ApJ...522L..53B and 2001ApJS..134..103B 2001ApJS..134..103B, Cl* IC 2391 CTIO NNN in Simbad. L : Lynga, 1959ArA.....2..379L 1959ArA.....2..379L Cl* IC 2391 L NN in Simbad H : Hogg, 1960PASP...72...85H 1960PASP...72...85H, Cl* IC 2391 H NN in Simbad SHJM : Stauffer et al., 1989ApJ...342..285S 1989ApJ...342..285S Cl* IC 2391 SHJM NN in Simbad Note (2): Note as follows: a = These stars have R-I inconsistent with cluster membership (see Fig. 6) b = Stars having (J-K), J values incompatible with the cluster main sequence. Note (3): Flags as follows: * = members for which spectral and timing analysis has been done using the EPIC/pn camera ? = suspected cluster member # = observed only by MOS1 and MOS2 Note (4): The Kolmogorov-Smirnov test is an confidence level of variability. variable : K-S>99%, marginally variable : K-S between 90% and 99% not variable : K-S <90% -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 09-Mar-2006
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