G111.7−2.1
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Cassiopeia A,
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3C461
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- Right Ascension: 23 23 26
- Declination: +58 48
- Size (/arcmin): 5
- Type: S
- Flux density at 1 GHz (/Jy): 2300
- Spectral Index: 0.77
Notes: Presumably the remnant of a late 17th century SN.
- Radio: Bright shell with compact knots and extended plateau of emission; shows secular decline.
- Optical: Fast knots and quasi-stationary flocculli, with many filaments at large radii, and NE ‘jet’.
- X-ray: Incomplete shell, with hard spectral component.
- Point sources: Central compact X-ray source.
- Distance: Optical expansion gives 3.3 kpc.
References:
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- Kassim et al. 1995, ApJ, 455, L59. VLA at 74 (25″) and 332 MHz (6″), including spectral index comparisons.
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- Anderson & Rudnick 1996, ApJ, 456, 234. VLA for spectral index comparisons.
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- Schwarz et al. 1997, A&AS, 123, 43. WSRT at 1.4 GHz (30″) for HI absorption.
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- O′Sullivan & Green 1999, MNRAS, 303, 575. Flux density changes at 13.5, 15.5 and 16.5 GHz.
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- Agüeros & Green 1999, MNRAS, 305, 957. 151 MHz observations for bulk expansion studies.
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- Gotthelf et al. 2001, ApJ, 552, L39. Chandra observations, showing outer shock.
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- Hwang et al. 2001, ApJ, 560, L175. Chandra observations of Doppler shifted lines.
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- Fesen et al. 2001, AJ, 122, 2644. HST observations.
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- Reynoso & Goss 2002, ApJ, 575, 871. VLA at 5 GHz (6.″0×6.″4) for H2CO absorption studies.
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- Krause et al. 2005, Science, 308, 1604. Spitzer light echoes from surroundings.
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- Kang [1;5A& Koo 2007, ApJS, 173, 85. High velocity HI.
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- Rho et al. 2008, ApJ, 673, 271. Spitzer observations.
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- Rest et al. 2008, ApJ, 681, L81. SN light echo.
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- Krause et al. 2008, Science, 320, 1195. SN light echo spectrum.
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- Helmboldt & Kassim 2009, AJ, 138, 838. Low radio frequency temporal variations.
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- Barlow et al. 2010, A&A, 518, L138. Herschel observations.
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- Patnaude et al. 2011, ApJ, 729, L28. Chandra observations of fading.
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- Rest et al. 2011, ApJ, 732, 3. SN light echo observations.
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- Fesen et al. 2011, ApJ, 736, 109. HST variability studies.
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- Besel & Krause 2012, A&A, 541, L3. IR light echoes.
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- Vogt et al. 2012, ApJ, 750, 155. Spitzer light echoes.
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- Asgekar et al. 2013, A&A, 551, L11. LOFAR of carbon recombination lines.
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- Yang et al. 2013, ApJ, 766, 44. Suzaku spectroscopy.
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- Rutherford et al. 2013, ApJ, 769, 64. Chandra spectroscopy.
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- Milisavljevic & Fesen 2013, ApJ, 772, 134. Optical spectroscopy for 3-D structure.
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- Koo et al. 2013, Science, 342, 1346. IR spectroscopy.
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- DeLaney et al. 2014, ApJ, 785, 7. VLA plus Pie Town at 74 MHz (9″) and comparison with higher frequencies.
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- Arendt et al. 2014, ApJ, 786, 55. Spitzer and Herschel IR observations.
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- Patnaude & Fesen 2014, ApJ, 789, 138. Multi-epoch optical and X-ray observations.
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- Lee et al. 2014, ApJ, 789, 7. Spitzer and CO observations.
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- Vinyaikin 2014, ARep, 58, 626. Time evolution of radio emission.
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- Alarie et al. 2014, MNRAS, 441, 2996. Optical imaging/spectroscopy, including distance from expansion.
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- Grefenstette et al. 2014, Nature, 506, 339. NuSTAR 44Ti observations.
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- Grefenstette et al. 2015, ApJ, 802, 15. NuSTAR observations.
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- Lee et al. 2015, ApJ, 808, 98. WISE, Spitzer and other IR observations.
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- Milisavljevic & Fesen 2015, Science, 347, 526. Near-IR observations.
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- Planck Collaboration: Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 7 frequencies between 30 and 353 GHz.
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- Kilpatrick et al. 2016, ApJ, 816, 1. CO observations, including broad lines.
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- Fesen & Milisavljevic 2016, ApJ, 818, 17. HST [SIII] and [SII] observations.
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- Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties).
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- Wang & Li 2016, ApJ, 825, 102. INTEGRAL observations.
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- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
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- Oonk et al. 2017, MNRAS, 465, 1066. LOFAR observations, including H and C lines, 33 to 78 MHz, including 69 MHz (9.″8×11.″2).
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- De Looze et al. 2017, MNRAS, 465, 3309. Spitzer and Herschel observations.
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- Trotter et al. 2017, MNRAS, 469, 1299. Time evolution of radio emission.
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- Grefenstette et al. 2017, ApJ, 834, 19. NuSTAR observations.
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- Sato et al. 2017, ApJ, 836, 225. Multi-epoch Chandra observations.
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- Salas et al. 2018, MNRAS, 475, 2496. LOFAR C recombination lines as 43, 54, 148 and 340 MHz (70″).
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- Sato et al. 2018, ApJ, 853, 46. Chandra and NuSTAR observations.
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- Zhou et al. 2018, ApJ, 865, 6. CO observations.
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- Raymond et al. 2018, ApJ, 866, 128. IR observations.
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- Koo et al. 2018, ApJ, 866, 139. IR observations.
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also see: Koo et al. 2020, ApJ, 896, 177. Erratum.
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- Chowdhury & Chengalur 2019, MNRAS, 486, 42. GMRT at 410 to 460 MHz for C recombination lines.
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- de Gasperin et al. 2020, A&A, 635, A150. LOFAR at 30 to 77 MHz (7″×10″).
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- Weinberger et al. 2020, A&A, 638, A83. INTEGRAL observations.
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- Koo et al. 2020, NatAs, 4, 584. Near IR spectroscopy of surroundings.
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- Weil et al. 2020, ApJ, 891, 116. Deep Hα of surroundings.
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- Mayer & Becker 2021, A&A, 651, A40. Multi-epoch Chandra observations for proper motion of compact source.
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- Domček et al. 2021, MNRAS, 502, 1026. Radio to IR spectral study.
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- Ikeda et al. 2022, PASJ, 74, 334. Chandra observations of NE.
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- Vink et al. 2022, ApJ, 929, 57. Multi-epoch Chandra observations for proper motion study.
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- Tsuchioka et al. 2022, ApJ, 932, 93. Chandra observations of SE.
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- Vink et al. 2022, ApJ, 938, 40. IXPE polarisation observations.
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- Lei et al. 2022, ApJ, 941, 13. Multi-epoch VLA observations of radio knots.
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- Stanislavsky et al. 2023, A&A, 670, A157. 15 to 72 MHz radio observations.
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- Koo et al. 2023, ApJ, 953, 131. Near-IR spectroscopy of knots in E.
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- Rho et al. 2023, MNRAS, 522, 2279. SOFIA far-IR polarisation observations.
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Last updated: 12 Mar 2024
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