J/A+A/299/39        Orion Trapezium area ROSAT PSPC obs. I.  (Geier+, 1995)

ROSAT PSPC observations of the Orion Trapezium area. I. Pre-main sequence and O stars. Geier S., Wendker H.J., Wisotzki L. <Astron. Astrophys. 299, 39 (1995)> =1995A&A...299...39G 1995A&A...299...39G
ADC_Keywords: Clusters, open ; X-ray sources ; Stars, pre-main sequence Mission_Name: ROSAT Keywords: early-type stars - pre-main sequence stars - ISM: bubbles - associations: Orion Trapezium - X-rays: stars Abstract: A deep ROSAT PSPC image centred on the Orion Trapezium has revealed that most of the X-ray emission originates from discrete sources, in contrast to previous EINSTEIN data which suggested a diffuse emission component. We present a list of 171 X-ray sources all situated in the so-called inner ring of the field of view (20' radius). The field is crowded with sources. A special procedure had to be developed to cope with the severe blending of sources. The present list is not complete for LX<3.5*1029erg/s due to this reason and many more sources can still be expected by a next step in the reduction. Nearly all of the sources could be identified with pre-main sequence stars of the Ori OB 1 association in its subgroups Ic and Id. The statistics of this ensemble are discussed. It seems that members of the above subgroups can be distinguished on the basis of an additional amount of X-ray extinction seen in their spectra or hardness ratios. The O stars in the area ({teta}1 Ori C, {teta}2 Ori A and ι Ori) are briefly discussed. Six B stars are identified with X-ray sources. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 73 171 Positions and identifications of X-ray sources table2.dat 38 171 X-ray properties of the sample -------------------------------------------------------------------------------- See also: IX/30 : Second ROSAT PSPC Catalog (ROSAT, 2000) IX/31 : The WGACAT version of ROSAT sources (White+ 2000) J/AN/321/81 : Orion Trapezium area ROSAT PSPC obs. II. (Lohmann+, 2000) J/ApJ/540/1016 : K-band & NICMOS phot. of Trapezium Cluster (Luhman+, 2000) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- ROS-ORI [1/171]+ Sequential number 5- 6 I2 h RAh Right ascension (J2000.0) 8- 9 I2 min RAm Right ascension (J2000.0) 11- 14 F4.1 s RAs Right ascension (J2000.0) 16 A1 --- DE- Declination sign (J2000.0) 17- 18 I2 deg DEd Declination (J2000.0) 20- 21 I2 arcmin DEm Declination (J2000.0) 23- 24 I2 arcsec DEs Declination (J2000.0) 26- 30 F5.2 arcmin phi Off-axis angle 32- 35 I4 --- P ? Parenago (1954TrSht..25....1P 1954TrSht..25....1P) number 37- 40 I4 --- JW ? Jones & Walker (1988AJ.....95.1755J 1988AJ.....95.1755J) number 42- 51 A10 --- Var Variable name 53- 82 A30 --- Names Other names -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- ROS-ORI [1/171]+ Sequential number 5- 9 I5 ct NPhot Net X-ray photon count 11- 17 F7.2 ct/ks CountRate Count rate 19- 23 F5.2 --- HR1 Hardness ratio HR1 25- 29 F5.2 --- HR2 Hardness ratio HR2 31- 33 F3.1 MK Tx ? Temperature of corona plasma 35- 38 F4.1 10+21cm-2 N(HI) ? HI column density -------------------------------------------------------------------------------- History: Prepared via OCR at CDS.
(End) James Marcout, Patricia Bauer [CDS] 05-Oct-2000
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