J/AJ/121/337        Chandra Observation of the Pleiades   (Krishnamurthi+, 2001)

Observations of the core of the Pleiades with the Chandra X-ray observatory. Krishnamurthi A., Reynolds C.S., Linsky J.L., Martin E., Gagne M. <Astron. J., 121, 337-346 (2001)> =2001AJ....121..337K 2001AJ....121..337K (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, open ; X-ray sources ; Stars, early-type ; Stars, late-type Mission_Name: Chandra Keywords: Galaxy: Open Clusters and Associations: Individual: Name: Pleiades, Stars: Activity, Stars: Early-Type, Stars: Low-Mass, Brown Dwarfs Abstract: We present results from a 36 ks observation of the core of the Pleiades open cluster using ACIS-I on the Chandra X-Ray Observatory. We have detected 57 sources, most of which do not have previously known optical counterparts. Follow-up photometry indicates that many of the detections are likely to be active galactic nuclei, in accordance with extragalactic source counts, but some of the sources may be previously undiscovered low-mass members of the Pleiades. We discuss our data set and our findings about X-ray emission from early-type stars, as well as very late-type stars. In particular, the large X-ray fluxes, lack of variability, and hardness ratios of the four Pleiades B6 IV-F4 V stars suggest a tentative conclusion that Pleiades stars in this spectral type range are intrinsic X-ray sources rather than previously unknown binaries in which the X-ray emission is from a late-type companion. Also, the sensitivity of Chandra allowed us to detect nonflare X-ray emission from late M stars. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 50 57 Sources Detected by Chandra table2.dat 41 18 Known Optical Counterparts to ACIS Detections -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Seq Source number 4 I1 h RAh Right ascension (J2000) 6- 7 I2 min RAm Right ascension (J2000) 9- 13 F5.2 s RAs Right ascension (J2000) 15- 16 I2 deg DEd Declination (J2000) 18- 19 I2 arcmin DEm Declination (J2000) 21- 25 F5.2 arcsec DEs Declination (J2000) 27- 33 F7.2 ct Counts Source counts 35- 39 F5.2 ct e_Counts Statistical error in Counts 41- 45 F5.2 --- HR Hardness ratio (1) 47- 50 F4.2 --- e_HR Uncertainty in HR -------------------------------------------------------------------------------- Note (1): HR = (hard - soft)/(hard + soft), where hard is from the 1-3keV image and soft is from the 0-1keV image. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Seq Source number 4- 11 A8 --- Opt Optical counterpart (1) 13 A1 --- f_Opt Indicates a star has flared during the observation. Discussion in sections 3.4 and 3.5. 15- 17 F3.1 arcsec Offset Offset from the optical counterpart 19- 22 F4.2 arcsec COffset Corrected offset from the optical counterpart 24- 27 I4 ct Counts X-ray counts 29- 33 F5.2 mag Vmag The V-band magnitude 35- 39 A5 --- SpType Spectral type 41 A1 --- Member Membership (2) -------------------------------------------------------------------------------- Note (1): HII = The second list in Hertzsprung 1947, sometimes also referred to as Hz (see e.g. Cat. I/90) HCG = The catalog of Haro, Chavira, & Gonzalez 1982 (Cat. II/131) HHJ = The Hambly, Hawkins, & Jameson catalog 1991 (J/A+AS/100/607) MHO = Objects from the Mount Hopkins survey (Stauffer et al. 1998ApJ...504..805S 1998ApJ...504..805S). Note (2): Y = Member; ? = Uncertain membership. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Laurent Cambresy [CDS] 17-Aug-2004
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