G347.3−0.5
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RX J1713.7−3946
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- Right Ascension: 17 13 50
- Declination: −39 45
- Size (/arcmin): 65×55
- Type: S?
- Flux density at 1 GHz (/Jy): 30?
- Spectral Index: ?
- Radio: Faint emission.
- X-ray: Non-thermal, limb-brightened to W, with central source.
- Point sources: Central X-ray source.
- Distance: Association with molecular clouds and X-ray observations imply 1.3 kpc, association with dust suggests 1.1 kpc, optical extinction suggests 4.6 kpc.
References:
- Koyama et al. 1997, PASJ, 49, L7. ASCA of NW.
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- Slane et al. 1999, ApJ, 525, 357. ASCA and other observations.
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- Muraishi et al. 2000, A&A, 354, L57. γ-ray detection.
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- Butt et al. 2001, ApJ, 562, L167. Associated γ-ray emission.
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- Ellison et al. 2001, ApJ, 563, 191. ATCA at 1.4 GHz (36″×46″), and ASCA observations.
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- Enomoto et al. 2002, Nature, 416, 823. γ-ray observations.
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- Uchiyama et al. 2002, PASJ, 54, L73. ASCA observations.
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- Uchiyama et al. 2003, A&A, 400, 567. Chandra spectroscopy.
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- Pannuti et al. 2003, ApJ, 593, 377. ROSAT, ASCA and RXTE observations.
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- Lazendic et al. 2003, ApJ, 593, L27. Chandra, XMM-Newton and other X-ray observations of central source.
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- Fukui et al. 2003, PASJ, 55, L61. CO observations of surroundings.
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- Cassam-Chenaï et al. 2004, A&A, 427, 199. XMM-Newton and other observations.
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- Aharonian et al. 2004, Nature, 432, 75. H.E.S.S. detection.
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- Lazendic et al. 2004, ApJ, 602, 271. Chandra observations of parts, and ATCA at 1.4 GHz (36″×46″).
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- Hiraga et al. 2005, A&A, 431, 953. XMM-Newton observations.
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- Moriguchi et al. 2005, ApJ, 631, 947. CO observations of surroundings.
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- Aharonian et al. 2007, A&A, 464, 235. H.E.S.S. observations.
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also see: Aharonian et al. 2011, A&A, 531, C1. Erratum.
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- Uchiyama et al. 2007, Nature, 449, 576. Chandra multi-epoch observations for study of small-scale variability.
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- Tanaka et al. 2008, ApJ, 685, 988. Suzaku observations.
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- Takahashi et al. 2008, PASJ, 60, S131. Suzaku observations of SW.
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- Mignani et al. 2008, A&A, 484, 457. Optical and IR observations of central source.
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- Acero et al. 2009, A&A, 505, 157. XMM-Newton observations, plus other radio, IR and H.E.S.S. observations.
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- Sano et al. 2010, ApJ, 724, 59. CO observations of region.
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- Maxted et al. 2012, MNRAS, 422, 2230. Molecular line observations.
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also see: Maxted et al. 2013, MNRAS, 430, 2511. Erratum.
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- Sano et al. 2013, ApJ, 778, 59. CO, SGPS HI and Suzaku observations.
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- Federici et al. 2015, A&A, 577, A12. Fermi detection.
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- Sano et al. 2015, ApJ, 799, 175. Suzaku observations.
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- Katsuda et al. 2015, ApJ, 814, 29. XMM-Newton observations.
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- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
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- Tsuji & Uchiyama 2016, PASJ, 68, 108. Chandra observations of NW.
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- Acero et al. 2017, A&A, 597, A106. XMM-Newton observations for proper motion studies.
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- Okuno et al. 2018, PASJ, 70, 77. Chandra observations.
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- H.E.S.S. Collaboration: Abdalla et al. 2018, A&A, 612, A6. H.E.S.S. observations.
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- Kuznetsova et al. 2019, MNRAS, 489, 1828. INTEGRAL observations.
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- Tsuji et al. 2019, ApJ, 877, 96. NuSTAR observations.
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- Higurashi et al. 2020, ApJ, 899, 102. Chandra of NW.
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- Tanaka et al. 2020, ApJ, 900, L5. Chandra of SW.
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- Sano et al. 2020, ApJ, 904, L24. ALMA CO observations.
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- Wang et al. 2020, A&A, 639, A72. Optical extinction for distance.
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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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- Fukui et al. 2021, ApJ, 915, 84. H.E.S.S. observations.
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- Tateishi et al. 2021, ApJ, 923, 187. XMM-Newton spectroscopy.
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- Leike et al. 2021, NatAs, 5, 832. Dust clouds, including distance.
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Last updated: 16 Dec 2022
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