Note: this is an archived version which has been superseded. The current SNR catalogue is at https://www.mrao.cam.ac.uk/surveys/snrs/

G120.1+1.4 ADS: search fulltext or title/keyword/abstract

Tycho, 3C10, SN1572

• Right Ascension: 00 25 18
• Declination: +64 09
• Size (/arcmin): 8
• Type: S
• Flux density at 1 GHz (/Jy): 50
• Spectral Index: 0.58

Notes: This is the remnant of the Tycho's SN of AD1572.

Radio: Shell, brightest to the NE.

Optical: Faint filaments/knots to the NNW, NE and E.

X-ray: Shell, brighter to the NE.

Point sources: Faint radio source near centre of the remnant, thought to be extragalactic.

Distance: HI observations suggest 2.3–3 kpc, optical proper motion and shock velocity gives 2.4 kpc.

References:

• Duin & Strom 1975, A&A, 39, 33. WSRT at 610 MHz (57''×64'') and 5 GHz (7''×8''). ADS
• Klein et al. 1979, A&A, 76, 120. Effelsberg 100-m at 10.7 GHz (1.'2: S=13.1±0.8 Jy), plus review of flux densities. ADS
• Strom et al. 1982, MNRAS, 200, 473. WSRT at 1415 MHz (27''×31'') from 1971 and 1979, for expansion. ADS
• Dickel et al. 1982, ApJ, 257, 145. Comparison of radio, X-ray and optical observations. ADS
• Seward et al. 1983, ApJ, 266, 287. Einstein observations. ADS
• Tan & Gull 1985, MNRAS, 216, 949. Radio at 2.7 GHz (4'') from 1980 and 1983, and One-Mile Telescope at 1.4 GHz (23'') from 1965 and 1980, for expansion. ADS
• Albinson et al. 1986, MNRAS, 219, 427. HI observations. ADS
• Green & Gull 1987, MNRAS, 224, 1055. VLA HI absorption observations towards central radio source. ADS
• Wood et al. 1992, AJ, 103, 1338. VLA at 5 GHz (1.''5) polarisation studies. ADS
• Vancura et al. 1995, ApJ, 441, 680. X-ray spectra and ROSAT image. ADS
• Predehl & Schmitt 1995, A&A, 293, 889. ROSAT of dust scattered halo. ADS
• Schwarz et al. 1995, A&A, 299, 193. WSRT and Effelsberg 100-m at 1.4 GHz (50''), and VLA at 1.4 GHz (13''), for neutral hydrogen studies. ADS
• Hwang & Gotthelf 1997, ApJ, 475, 665. ASCA observations. ADS
• Reynoso et al. 1997, ApJ, 491, 816. VLA at 1.4 GHz (1.''4×1.''5) from 1984 and 1994 for expansion studies. ADS
• Lorimer et al. 1998, A&A, 331, 1002. Pulsar search. ADS
• Reynoso et al. 1999, AJ, 117, 1827. VLA at 1.4 GHz (13''), for HI studies. ADS
• Katz-Stone et al. 2000, ApJ, 529, 453. VLA at 333 MHz and 1.4 GHz (7.''7×9.''5), for spectral index studies. ADS
• Hughes 2000, ApJ, 545, L53. ROSAT X-ray expansion. ADS
• Decourchelle et al. 2001, A&A, 365, L218. XMM-Newton observations. ADS
• Ghavamian et al. 2001, ApJ, 547, 995. Optical spectroscopy. ADS
• Douvion et al. 2001, A&A, 373, 281. ISO observations. ADS
• Lee et al. 2004, ApJ, 605, L113. Observations of molecular clouds in vicinity. ADS
• Warren et al. 2005, ApJ, 634, 376. Chandra observations. ADS
• Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=86±5 Jy) and 1420 MHz (~1': S=40.5±1.5 Jy), including polarisation and review of flux densities. ADS
• Cassam-Chenaï et al. 2007, ApJ, 665, 315. Chandra observations. ADS
• Rest et al. 2008, ApJ, 681, L81. SN light echo. ADS
• Krause et al. 2008, Nature, 456, 617. SN light echo spectrum. ADS
• Hurley-Walker et al. 2009, MNRAS, 396, 365. Radio observations at 14 to 18 GHz. ADS
• Raymond et al. 2010, ApJ, 712, 901. Hα spectroscopy. ADS
• Lee et al. 2010, ApJ, 715, L146. Hα observations. ADS
• Hayato et al. 2010, ApJ, 725, 894. Suzaku observations of expansion. ADS
• Ishihara et al. 2010, A&A, 521, L61. Akari observations. ADS
• Tian & Leahy 2011, ApJ, 729, L15. HI and CO observations. ADS
• Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=20.0±2.0 Jy) including polarisation and review of flux densities. ADS
• Giordano et al. 2012, ApJ, 744, L2. Fermi observations. ADS
• Gomez et al. 2012, MNRAS, 420, 3557. Herschel IR dust observations. ADS
• Williams et al. 2013, ApJ, 770, 129. Spitzer observations. ADS
• Wang & Li 2014, ApJ, 789, 123. INTEGRAL observations. ADS
• Troja et al. 2014, ApJ, 797, L6. Swift observations. ADS
• Miceli et al. 2015, ApJ, 805, 120. XMM-Newton observations. ADS
• Lu et al. 2015, ApJ, 805, 142. Chandra observations. ADS
• Katsuda et al. 2015, ApJ, 808, 49. Suzaku observations. ADS
• Tran et al. 2015, ApJ, 812, 101. Chandra observations. ADS
• Lopez et al. 2015, ApJ, 814, 132. NuSTAR observations. ADS
• Planck Collaboration: Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 5 frequencies between 30 and 143 GHz. ADS
• Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties). ADS
• Williams et al. 2016, ApJ, 823, L32. Multi-epoch X-ray and radio observations for expansion. ADS
• Zhou et al. 2016, ApJ, 826, 34. CO observations. ADS
• Chen et al. 2017, A&A, 604, A13. CO observations. ADS
• Yamaguchi et al. 2017, ApJ, 834, 124. Suzaku observations of E rim. ADS
• Archambault et al. 2017, ApJ, 836, 23. γ-ray observations. ADS
• Sato & Hughes 2017, ApJ, 840, 112. Chandra and Suzaku observations. ADS
• Williams et al. 2017, ApJ, 842, 28. Multi-epoch Chandra observations for expansion studies. ADS
• Knežević et al. 2017, ApJ, 846, 167. Hα observations of NE. ADS
• Kerzendorf et al. 2018, MNRAS, 479, 5696. HST search for progenitor companion. ADS
• Vinyaikin et al. 2018, ARep, 62, 130. Time evolution of radio emission. ADS
• Arias et al. 2019, AJ, 158, 253. LOFAR at 58 (41'') and 143 MHz (6''). ADS
• Weinberger et al. 2020, A&A, 638, A83. INTEGRAL observations. ADS
• Matsuda et al. 2020, PASJ, 72, 85. Multi-epoch Chandra study. ADS
• Okuno et al. 2020, ApJ, 894, 50. Multi-epoch Chandra study. ADS
• Williams et al. 2020, ApJ, 898, L51. XMM-Newton spectroscopy. ADS
• Castelletti et al. 2021, A&A, 653, A62.VLA 74-MHz survey flux density. ADS
• Millard et al. 2021, ApJS, 257, 36. ISO far-IR spectroscopy. ADS
• Tanaka et al. 2021, ApJ, 906, L3. Multi-epoch Chandra observations for expansion. ADS

Last updated: 16 Dec 2022

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