J/A+A/394/975       OH 5-cm line survey in late-type stars      (Desmurs+, 2002)

A high-sensitivity OH 5-cm line survey in late-type stars Desmurs J.-F., Baudry A., Sivagnanam P., Henkel C. <Astron. Astrophys. 394, 975 (2002)> =2002A&A...394..975D 2002A&A...394..975D
ADC_Keywords: Masers ; Surveys ; Stars, late-type ; Stars, giant ; Radio sources Keywords: masers - stars: AGB and post-AGB - radio lines: stars Abstract: We have undertaken a comprehensive search for 5-cm excited OH maser emission from evolved stars representative of various stages of late stellar evolution. Observed sources were selected from known 18-cm OH sources. This survey was conducted with the 100-m Effelsberg telescope, at 6.0GHz in Sep 2000, to achieve high signal to noise ratio observations and a sensitivity limit of about 0.05 to 0.1Jy. A total of 65 stellar sources were searched for both main line and satellite line emission. We confirm the previous detection of 5 cm OH in Vy 2-2, do not confirm emission from NML-Cyg and do not report any other new detection within the above sensitivity limit. The number of observed sources is 67. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 93 67 Observations of the 6GHz OH maser transitions in AGB stars table1.tex 107 135 LaTeX version of table1 -------------------------------------------------------------------------------- See also: V/18 : Catalogue of Late-type Stars with Maser Emission (Engels 1979) J/A+A/277/453 : OH maser survey of cool IRAS sources (David+ 1993) J/A+A/325/255 : 5cm OH masers survey (Baudry+ 1997) J/A+AS/119/459 : Search for OH maser emission from post-AGB (te Lintel Hekkert+ 1996) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- IRAS IRAS name of the source 13- 25 A13 --- Name Alternative source name 27- 41 A15 --- Type Source type (1) 43- 44 I2 h RAh Right ascension (J2000.0) (2) 46- 47 I2 min RAm Right ascension (J2000.0) 49- 54 F6.3 s RAs Right ascension (J2000.0) 56 A1 --- DE- Declination sign (J2000.0) 57- 58 I2 deg DEd Declination (J2000.0) 60- 61 I2 arcmin DEm Declination (J2000.0) 63- 67 F5.2 arcsec DEs Declination (J2000.0) 70- 73 I4 km/s Vel1 Lower limit of the observed velocity Range 74 A1 --- --- [/] 75- 78 I4 km/s Vel2 Upper limit of the observed velocity Range 81- 85 F5.1 km/s RVlsr LSR radial velocity 88 A1 --- n_Sen [E] E = Emission 89 A1 --- --- [/] 90- 93 F4.2 Jy Sen ? Sensitivity at 6GHz (3) -------------------------------------------------------------------------------- Note (1): The following abbreviations are used: UCHII: Ultra Compact HII region SG: Supergiant SR: Semi-regular variable PN: Planetary nebula PPN: Proto-planetary nebula Note (2): B1950 coordinates processed to J2000 within GILDAS package Note (3): The upper limits correspond to 3σ -------------------------------------------------------------------------------- Acknowledgements: Jean-Francois Desmurs
(End) Patricia Bauer [CDS] 28-Aug-2002
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