G348.7+0.3
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CTB 37B
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- Right Ascension: 17 13 55
- Declination: −38 11
- Size (/arcmin): 17?
- Type: S
- Flux density at 1 GHz (/Jy): 26
- Spectral Index: 0.3
- Radio: Incomplete shell with faint eastern extensions.
- X-ray: Diffuse emission.
- Point sources: X-ray pulsar.
- Distance: HI absorption suggests 9.8 kpc.
References:
- Clark et al. 1975, AuJPA, 37, 75. Molonglo at 408 MHz (3′: S=34 Jy).
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- Milne & Dickel 1975, AuJPh, 28, 209. Parkes 64-m at 5 GHz (4.′4: S=32 Jy).
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- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
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- Milne et al. 1979, MNRAS, 188, 437. FIRST at 1415 MHz (0.′8: S>20) and Parkes 64-m at 14.7 GHz (2.′2: S=8±3 Jy).
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- Downes 1984, MNRAS, 210, 845. VLA at 1465 MHz (20″×45″).
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- Kassim et al. 1991, ApJ, 374, 212. VLA at 333 MHz (46″×53″).
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- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43″×69″: S=33 Jy).
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- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant.
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- Aharonian et al. 2006, ApJ, 636, 777. H.E.S.S. detection.
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- Aharonian et al. 2008, A&A, 486, 829. H.E.S.S. and Chandra observations.
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- Nakamura et al. 2009, PASJ, 61, S197. Suzaku and Chandra observations.
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- Halpern & Gotthelf 2010, ApJ, 710, 941. Chandra detection of pulsar.
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- Halpern & Gotthelf 2010, ApJ, 725, 1384. Chandra observations of pulsar.
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- Tian & Leahy 2012, MNRAS, 421, 2593. SGPS HI observations.
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- Xin et al. 2016, ApJ, 817, 64. Fermi observations.
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- Blumer et al. 2019, MNRAS, 487, 5019. XMM-Newton, Chandra and HI observations.
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- Watanabe et al. 2019, PASJ, 71, 84. XMM-Newton observations of pulsar.
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- Gotthelf et al. 2019, ApJ, 882, 173. Chandra, XMM-Newton and NuSTAR observations of pulsar.
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- Chawner et al. 2020, MNRAS, 493, 2706. Herschel observations.
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Last updated: 9 Dec 2022
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