G74.0−8.5
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Cygnus Loop
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- Right Ascension: 20 51 00
- Declination: +30 40
- Size (/arcmin): 230×160
- Type: S
- Flux density at 1 GHz (/Jy): 210
- Spectral Index: varies
Notes: Has been suggested that this is two overlapping remnants.
- Radio: Shell, brightest to the NE, with fainter breakout region to S, with spectral variations.
- Optical: Large filamentary loop, brightest to the NE, not well defined to the S or W.
- X-ray: Shell in soft X-rays.
- Point sources: Several compact radio sources within the boundary of the remnant.
- Distance: Stellar interactions gives 0.73 kpc.
References:
- Green 1990, AJ, 100, 1927. DRAO at 408 MHz (3.′3×6.′7) for spectral index study, plus X-ray and optical.
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- Graham et al. 1991, AJ, 101, 175. Shocked molecular H outside rim in NE.
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- Fesen et al. 1992, AJ, 104, 719. Hα imagery.
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- Arendt et al. 1992, ApJ, 400, 562. IRAS observations.
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- Hester et al. 1994, ApJ, 420, 721. Hα, [OIII] and other optical observations of Balmer dominated filaments in NE.
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- Gorham et al. 1996, ApJ, 458, 257. Pulsar search.
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- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
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- Leahy et al. 1997, AJ, 114, 2081. DRAO at 1.4 GHz (1′×2′), including polarisation.
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- Leahy & Roger 1998, ApJ, 505, 784. DRAO at 1.4 GHz (1.′0×1.′9) and 408 MHz (3.′4×6.′9), for spectral index studies in comparison with other radio observations.
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- Levenson et al. 1998, ApJS, 118, 541. Optical images.
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- Roger et al. 1999, A&AS, 137, 7. 22 MHz flux density (S=1400±400 Jy).
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- Bohigas et al. 1999, ApJ, 518, 324. Optical spectroscopy of surroundings.
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- Levenson et al. 1999, ApJ, 526, 874. ROSAT images.
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- Blair et al. 1999, AJ, 118, 942. HST observations, for distance.
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- Danforth et al. 2000, AJ, 119, 2319. UV, optical and X-ray comparison of selected regions.
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- Miyata et al. 2001, ApJ, 550, 1023. ASCA observations of compact X-ray sources.
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- Danforth et al. 2001, AJ, 122, 938. Far-UV spectroscopy, Hα and other optical observations of NE region.
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- Levenson & Graham 2001, ApJ, 559, 948. HST of SE region.
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- Uyanıker et al. 2002, A&A, 389, L61. Effelsberg 100-m at 2.7 GHz (4.′3) including polarisation, and comparison with ROSAT data.
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- Leahy 2002, AJ, 123, 2689. DRAO at 1.4 GHz (2′×4′) for HI.
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- Blair et al. 2002, ApJS, 140, 367. UV spectroscopy.
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- Levenson et al. 2002, ApJ, 576, 798. Chandra observations of W edge.
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- Reich et al. 2003, A&A, 408, 961. Effelsberg 100-m at 863 MHz (14.′5: S=184±18 Jy).
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- Leahy 2004, MNRAS, 351, 385. Chandra observations of SW.
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- Uyanıker et al. 2004, A&A, 426, 909. Effelsberg 100-m at 2.7 GHz (4.′3), with comparison with other data for spectral index studies.
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- Blair et al. 2005, AJ, 129, 2268. HST of outer filaments.
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- Leahy 2005, AJ, 130, 165. DRAO at 1.4 GHz of SE.
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- Levenson & Graham 2005, ApJ, 622, 366. Chandra observations of knot in SE.
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- Sun et al. 2006, A&A, 447, 937. Urumqi 25-m at 4.8 GHz (9.′5: S=90±9 Jy), with comparisons with other data for spectral index studies.
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- Kaplan et al. 2006, ApJS, 163, 344. X-ray upper limit on compact sources.
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- Seon et al. 2006, ApJ, 644, L175. Far UV observations.
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- Sankrit et al. 2007, AJ, 133, 1383. UV observations of part.
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- Tsunemi et al. 2007, ApJ, 671, 1717. XMM-Newton observations of NE to SW.
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- Nemes et al. 2008, ApJ, 675, 1293. XMM-Newton observations of NE.
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- Katsuda et al. 2008, ApJ, 680, 1198. Chandra observations of NE.
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- Uchida et al. 2008, ApJ, 688, 1102. XMM-Newton observations.
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- Uchida et al. 2009, PASJ, 61, 503. Suzaku observations of N.
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- Kimura et al. 2009, PASJ, 61, S137. Suzaku observations from NE to SW.
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- Tsunemi et al. 2009, PASJ, 61, S147. Suzaku observations of SE.
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- Kosugi et al. 2010, PASJ, 62, 1035. Suzaku observations of SE.
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- Sankrit et al. 2010, ApJ, 712, 1092. Spitzer observations.
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- McEntaffer & Brantseg 2011, ApJ, 730, 99. Chandra observations of E.
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- Katagiri et al. 2011, ApJ, 741, 44. Fermi observations.
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- Leahy & Hassan 2013, ApJ, 764, 55. Suzaku and XMM-Newton observations of SW.
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- Oakley et al. 2013, ApJ, 766, 51. X-ray spectroscopy.
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- Kim et al. 2014, ApJ, 784, 12. Far UV observations.
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- Sankrit et al. 2014, ApJ, 787, 3. Spitzer spectroscopy in SE.
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- Medina et al. 2014, ApJ, 791, 30. Optical spectroscopy in NE.
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- Raymond et al. 2015, ApJ, 805, 152. HST observations in NE.
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also see: Raymond et al. 2015, ApJ, 814, 165. Erratum.
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- Roberts & Wang 2015, MNRAS, 449, 1340. Suzaku observations.
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- Planck Collaboration: Arnaud et al. 2016, A&A, 586, A134. Planck flux density 30 GHz.
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- Katsuda et al. 2016, ApJ, 819, L32. Hα spectroscopy of NE.
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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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- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
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- Boubert et al. 2017, A&A, 606, A14. Gaia search for runaway progenitor companion.
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- Seok et al. 2020, ApJ, 893, 79. Optical spectroscopy.
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- Raymond et al. 2020, ApJ, 903, 2. Optical spectroscopy.
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- Fesen et al. 2021, MNRAS, 507, 244. Gaia observations for distance.
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- Sun et al. 2022, RAA, 22, 125011. FAST at 1.27 GHz (4′), including polarisation.
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- Sankrit et al. 2023, ApJ, 948, 97. Multi-epoch HST observations.
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- Raymond et al. 2023, ApJ, 954, 34. Optical spectroscopy and proper motion study of filaments in E.
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Last updated: 12 Mar 2024
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