G320.4−1.2
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MSH 15−52,
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RCW 89
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- Right Ascension: 15 14 30
- Declination: −59 08
- Size (/arcmin): 35
- Type: C
- Flux density at 1 GHz (/Jy): 60?
- Spectral Index: 0.4
Notes: Has been suggested as the remnant of the SN of AD185?
- Radio: Ragged shell.
- Optical: RCW 89 is the Hα emitting region to the NW.
- X-ray: Partial shell, central nebula and pulsar and ‘jet’.
- Point sources: Radio and X-ray pulsar, with wind nebula.
- Distance: HI absorption indicates 5.2 kpc, optical extinction suggests 3.0 kpc.
References:
- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
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- Dickel & Milne 1976, AuJPh, 29, 435. Comparison of earlier Parkes 64-m maps at 2.7 GHz (8.′4) and 5 GHz (4.′4).
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- Dopita et al. 1977, ApJ, 214, 179. Optical spectra.
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- Caswell et al. 1981, MNRAS, 195, 89. FIRST at 1415 MHz (50″).
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- Seward & Harnden 1982, ApJ, 256, L45. X-ray observations of pulsar.
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- Manchester et al. 1982, ApJ, 262, L31. Radio observations of pulsar.
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- Seward et al. 1983, ApJ, 267, 698. X-ray, Optical and IR.
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- van den Bergh & Kamper 1984, ApJ, 280, L51. Optical expansion.
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- Seward et al. 1984, ApJ, 281, 650. X-ray observations of pulsar and nebulosity.
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- Lortet et al. 1987, A&A, 180, 65. Optical observations.
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- Trussoni et al. 1990, A&A, 234, 403. EXOSAT observations.
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- Asaoka & Koyama 1990, PASJ, 42, 625. Ginga X-ray spectrum.
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- Arendt 1991, AJ, 101, 2160. IRAS observations, including compact source.
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- Milne et al. 1993, MNRAS, 264, 853. Parkes 64-m at 4.8 GHz (4.′5: S=37±7 Jy) and 8.4 GHz (3.′0: S=24±4 Jy), including polarisation and review of flux densities.
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- Strom 1994, MNRAS, 268, L5. Historical association.
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- Chin & Huang 1994, Nature, 371, 398. Questioning of historical association.
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- Matz et al. 1994, ApJ, 434, 288. X-ray observations of pulsar.
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- Schaefer 1995, AJ, 110, 1793. Questioning of historical association.
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- Du Plessis et al. 1995, ApJ, 453, 746. Hartesbeesthoek 26-m at 2.3, 5 and 8.5 GHz (S=42, 35.6 and 14.5 Jy).
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- Greiveldinger et al. 1995, ApJ, 454, 855. ROSAT observations.
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- Trussoni et al. 1996, A&A, 306, 581. ROSAT observations.
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- Tamura et al. 1996, PASJ, 48, L33. ASCA observations.
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- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43″×50″: S=62 Jy).
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- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
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- Marsden et al. 1997, ApJ, 491, L39. X-ray spectroscopy.
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- Brazier & Becker 1997, MNRAS, 284, 335. ROSAT observations.
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- Gaensler et al. 1999, MNRAS, 305, 724. ATCA at 1.4 GHz (21″×24″), plus HI observations, and 5.3 GHz (10″×15″).
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- Sako et al. 2000, ApJ, 537, 422. Possible γ-ray detection of pulsar.
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- Mineo et al. 2001, A&A, 380, 695. BeppoSAX observations.
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- Gaensler et al. 2002, ApJ, 569, 878. Chandra observations of pulsar and nebula.
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- Dubner et al. 2002, AJ, 123, 337. ATCA at 1.4 GHz (2.′7×4.′0), plus HI observations.
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- Aharonian et al. 2005, A&A, 435, L17. H.E.S.S. detection.
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- Yatsu et al. 2005, ApJ, 631, 312. Chandra observations of pulsar and jet.
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- DeLaney et al. 2006, ApJ, 640, 929. Chandra and ROSAT multi-epoch observations of pulsar wind nebula.
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- Kaplan & Moon 2006, ApJ, 644, 1056. Possible IR detection of pulsar.
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- Forot et al. 2006, ApJ, 651, L45. X-ray observations of pulsar and nebula.
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- Nakamori et al. 2008, ApJ, 677, 297. γ-ray observations.
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- Yatsu et al. 2009, PASJ, 61, 129. Chandra observations of pulsar wind nebula.
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- Koo et al. 2011, ApJ, 732, 6. Akari and Spitzer observations.
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- An et al. 2014, ApJ, 793, 90. NuSTAR observations of PWN.
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- H.E.S.S. Collaboration: Abdalla et al. 2018, A&A, 612, A1. H.E.S.S. observations.
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- Borkowski et al. 2020, ApJ, 895, L32. Chandra observations.
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- Wang et al. 2020, A&A, 639, A72. Optical extinction for distance.
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- Millard et al. 2021, ApJS, 257, 36. ISO far-IR spectroscopy.
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Last updated: 15 Dec 2022
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