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J/A+A/333/619     Upper Scorpius OB association Lithium survey (Preibisch+ 1998)

A lithium-survey for pre-main sequence stars in the upper Scorpius OB association Preibisch T., Guenther E., Zinnecker H., Sterzik M., Frink S., Roeser S. <Astron. Astrophys. 333, 619 (1998)> =1998A&A...333..619P (SIMBAD/NED BibCode)
ADC_Keywords: Stars, pre-main sequence ; Equivalent widths ; Proper motions ; Associations, stellar Keywords: surveys - stars: kinematics - stars: pre-main sequence - open clusters and associations: Scorpius Centaurus - X-rays: stars Abstract: We present the results of an intermediate resolution spectroscopic survey for pre-main sequence (PMS) stars in the Upper Scorpius OB association. In a 160 square-degree area we were able to identify 39 new PMS stars by follow up observations of X-ray selected stars with the multi object spectrograph FLAIR at the UK Schmidt Telescope. We also investigated the completeness of our X-ray selected sample by observing more than 100 stars that were not detected as X-ray sources, but have proper motions indicating membership to Upper Sco. While the new X-ray selected PMS stars with known proper motions have kinematics consistent with membership, none of the X-ray quiet proper motion candidates is a PMS star. We conclude that our X-ray selected sample of PMS stars seems to be rather complete. For stars in the magnitude interval 11.5≲B≲13.5 we derive a conservative lower limit of 75% completeness. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablea1.dat 79 78 Results for the X-ray selected PMS candidates tablea2.dat 72 115 Results for the proper motion selected PMS candidates
Byte-by-byte Description of file: tablea1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- GSC GSC (Cat. I/220) number 11 A1 --- Index See Note (1) 13- 14 I2 h RAh Right ascension (J2000) 16- 17 I2 min RAm Right ascension (J2000) 19- 22 F4.1 s RAs Right ascension (J2000) 25 A1 --- DE- Declination sign 26- 27 I2 deg DEd Declination (J2000) 29- 30 I2 arcmin DEm Declination (J2000) 32- 33 I2 arcsec DEs Declination (J2000) 36- 39 F4.1 mag Bmag B magnitude from GSC (Cat. I/220) 42- 46 F5.3 ct/s CR ROSAT count rate 49 A1 --- u_CR [:<] Uncertainty/upper limit note (2) 50- 53 F4.2 0.1nm W(Li) Li line equivalent width 54 A1 --- u_W(Li) [:<] Uncertainty/upper limit note (2) 56- 61 F6.2 0.1nm W(Ha) Hα line equivalent width 63- 64 A2 --- SpType Spectral type 65 A1 --- u_SpType Uncertainty flag on SpType 67- 69 A3 --- Type See Note (3) 71- 74 I4 mas/yr pmRA ? Proper motion in right ascension *cos(delta) 76- 78 I3 mas/yr pmDE ? Proper motion in declination
Note (1): empty: X-ray source detected in the ROSAT All Sky Survey P: X-ray source detected in pointed ROSAT observation only Note (2): "<": Upper limit to the line width ":": Uncertainty exceeding 15% Note (3): Classification of the objects PMS: pre-main sequence star YC: non-PMS star with a Lithium line as typical for stars in the young clusters mentioned in Section 4 F: non-PMS star with a very weak lithium line (probably active field star)
Byte-by-byte Description of file: tablea2.dat
Bytes Format Units Label Explanations
1- 9 A9 --- GSC GSC (Cat. I/220) number 12- 13 I2 h RAh Right ascension (J2000) 15- 16 I2 min RAm Right ascension (J2000) 18- 21 F4.1 s RAs Right ascension (J2000) 24 A1 --- DE- Declination sign 25- 26 I2 deg DEd Declination (J2000) 28- 29 I2 arcmin DEm Declination (J2000) 31- 32 I2 arcsec DEs Declination (J2000) 36- 39 F4.1 mag Bmag B magnitude from GSC 42 A1 --- u_Bmag [:<] Uncertainty/upper limit note (1) 43- 46 F4.2 0.1nm W(Li) Li line equivalent width 47 A1 --- u_W(Li) [:<] Uncertainty/upper limit note (1) 50- 53 F4.2 0.1nm W(Ha) Hα line equivalent width 56- 57 A2 --- SpType Spectral type 58 A1 --- u_SpType Uncertainty flag on SpType 60- 61 A2 --- Type See Note (2) 64- 66 I3 mas/yr pmRA Proper motion in right ascension *cos(delta) 69- 71 I3 mas/yr pmDE Proper motion in declination
Note (1): <": Upper limit to the line width ":": Uncertainty exceeding 15% Note (2): Classification of the objects YC: non-PMS star with a Lithium line as typical for stars in the young clusters mentioned in Section 4 F: non-PMS star with a very weak lithium line (probably active field star)
Acknowledgements: Thomas Preibisch
(End) Patricia Bauer [CDS] 13-Feb-1998
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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