Search catalogue
J/MNRAS/329/775 330MHz flux of 4 SNR near Galactic Centre (Roy+, 2002)
GMRT observations of four suspected supernova remnants near the Galactic Centre. Roy S., Rao A.P. <Mon. Not. R. Astron. Soc. 329, 775 (2002)> =2002MNRAS.329..775R
ADC_Keywords: Supernova remnants ; Radio sources Keywords: ISM: individual: G3.1-0.6 - ISM: individual: G356.3-0.3 - ISM: individual: G356.6+0.1 - ISM: individual: G357.1-0.2 - supernova remnants - Galaxy centre Abstract: We have observed two fields - Field I (l=3.2°, b=1.0°) and Field II (l=356.8°, b=-0.1°) - with the Giant Metrewave Radio Telescope (GMRT) at 330MHz. In the first field, we have studied the candidate supernova remnant (SNR) G3.1-0.6 and, based on its observed morphology, spectral index and polarization, confirmed it to be an SNR. We find this supernova to have a double ring appearance with a strip of emission on its western side passing through its centre. We have discovered two extended curved objects in the second field, which appears to be part of a large shell-like structure. It is possibly the remains of an old supernova in the region. Three suspected SNRs, G356.3-0.3, G356.6+0.1 and G357.1-0.2, detected in the MOST 843-MHz survey of the GC region appear to be located on this shell-like structure. While both G356.3-0.3 and G356.6+0.1 seem to be parts of this shell, G357.1-0.2, which has a steeper spectrum above 1GHz, could be a background SNR seen through the region. Our Hi absorption observation towards the candidate SNR G357.1-0.2 indicates that it is at a distance of more than 6kpc from us. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 78 44 Compact sources in the field centred on G3.2-1.0 table5.dat 84 23 Compact sources in the field centred on G356.8-0.1
Table 1: Details of our observations -------------------------------------------------------------------------------- Galactic coord. RA (J2000) DE Frequency Date Obs. Available pointing center (MHz) Time (h) antennas -------------------------------------------------------------------------------- 003.2-0.1 17 57 00.1 -26 40 01 330 1999 Jun 25 6 27 356.8-0.1 17 38 11.4 -31 42 26 330 1999 Aug 01 3.5 24 357.2-0.2 17 39 40.6 -31 28 01 1420.6 2000 Feb 26 3.5 15 356.9+0.1 17 37 44.2 -31 31 15 1420.3 2000 Oct 07 0.5 26 Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 13 A13 --- [RR2002] Object Galactic coordinates 15- 16 I2 h RAh Right ascension (J2000.0) 18- 19 I2 min RAm Right ascension (J2000.0) 21- 24 F4.1 s RAs Right ascension (J2000.0) 26 A1 --- DE- Declination sign (J2000.0) 27- 28 I2 deg DEd Declination (J2000.0) 30- 31 I2 arcmin DEm Declination (J2000.0) 33- 34 I2 arcsec DEs Declination (J2000.0) 36- 40 F5.3 Jy Peak Peak flux at 330MHz (in Jy/beam) 42- 46 F5.3 Jy S0.33GHz Total flux density at 330MHz 48 A1 --- l_S1.4GHz Limit flag on S1.4GHz 49- 54 F6.4 Jy S1.4GHz Total flux density at 1.4GHz 57- 61 F5.2 arcmin Dist Distance from center (G3.2-1.0) 63- 78 A16 --- Com Comments (G1)
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 13 A13 --- [RR2002] Object Galactic coordinates 15- 16 I2 h RAh Right ascension (J2000.0) 18- 19 I2 min RAm Right ascension (J2000.0) 21- 24 F4.1 s RAs Right ascension (J2000.0) 26 A1 --- DE- Declination sign (J2000.0) 27- 28 I2 deg DEd Declination (J2000.0) 30- 31 I2 arcmin DEm Declination (J2000.0) 33- 34 I2 arcsec DEs Declination (J2000.0) 36- 40 F5.3 Jy Peak Peak flux at 330MHz (in Jy/beam) 42- 46 F5.3 Jy S0.33GHz Total flux density at 330MHz 48 A1 --- l_S1.4GHz Limit flag on 1.4GHz 49- 54 F6.4 Jy S1.4GHz Total flux density at 1.4GHz 55- 58 A4 --- n_S1.4GHz [(NV) ] NV: 1.4-GHz flux quoted from the NVSS 61- 67 F7.4 Jy S5GHz ? Flux density at 5GHz (G356.8-0.1) 69- 73 F5.2 arcmin Dist Distance from center 75- 84 A10 --- Com Comments (G1)
Global notes: Note (G1): TX denotes flux as measured by the Texas Survey at 365MHz. NV denotes flux at 1.4GHz from the NVSS
History: From electronic version of the journal
(End) James Marcout, Patricia Bauer [CDS] 22-Mar-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 |
© UDS/CNRS