Note: this is an
archived version which has been superseded. The current SNR
catalogue is at
http://www.mrao.cam.ac.uk/surveys/snrs/
G21.5-0.9
- Right Ascension: 18 30 47
- Declination: -10 37
- Size (arcmin): 1.2
- Type: F
- Flux density at 1 GHz (Jy): 6
- Spectral Index: 0.0
- Radio: Filled-centre, with high frequency turnover.
- X-ray: Detected, with power-law spectrum.
- Distance: HI absorption indicates 5.5 kpc.
References:
- Wilson & Weiler 1976, A&A, 53, 89. WSRT at 5 GHz (6"×35").
ADS
- Becker & Kundu 1976, ApJ, 204, 427. NRAO interferometer at 2.7 GHz (20"×5") and 8 GHz (7"×2"),
plus review of flux densities.
ADS
- Altenhoff et al. 1979, A&AS, 35, 23. Effelsberg 100-m at 4.9 GHz (2'.6).
ADS
- Becker & Szymkowiak 1981, ApJ, 248, L23. VLA at 5 GHz (8"), and HRI and IPC observations.
ADS
- Davelaar et al. 1986, ApJ, 300, L59. EXOSAT X-ray spectrum, and VLA HI observations.
ADS
- Morsi & Reich 1987, A&AS, 69, 533. Effelsberg 100-m at 32 GHz (26".5: S=5.64±0.29).
ADS
- Fürst et al. 1988, PASJ, 40, 347. NRO array at 22.3 GHz (4".4×7".3).
ADS
- Salter et al. 1989, A&A, 225, 167. Observations at 90.7 (29".5: S=3.8±0.4) and 141.9 GHz (S=2.5±1.2).
ADS
- Salter et al. 1989, ApJ, 338, 171. NRAO 12-m at 84.2 GHz (S=3.94±0.70), plus review of flux densities.
ADS
- Asaoka & Koyama 1990, PASJ, 42, 625. Ginga X-ray spectrum.
ADS
- Kassim 1992, AJ, 103, 943. VLA at 327 MHz (3'.3×3'.4: S=9).
ADS
- Wallace et al. 1994, A&A, 286, 565. HI of surroundings.
ADS
Last updated: 01 JUL 1995
Dave Green/MRAO, Cambridge, UK/D.A.Green@mrao.cam.ac.uk