SNR G116.6-26.1 , the SIMBAD biblio

SNR G116.6-26.1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST11:03:21


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Title First 3 Authors
2021MNRAS.507..971C 1130 T   A D     X C F     25 8 10 SRG/eROSITA discovery of a large circular SNR candidate
G116.6-26.1: SN Ia explosion probing the gas of the Milky Way halo?
CHURAZOV E.M., KHABIBULLIN I.I., BYKOV A.M., et al.
2022MNRAS.513L..83C 1515 T   A S   X C F     32 7 3 LOFAR detection of faint radio emission from the supernova remnant
SRGe J0023+3625 =
G116.6-26.1: probing the Milky Way synchrotron halo.
CHURAZOV E.M., KHABIBULLIN I.I., BYKOV A.M., et al.
2022MNRAS.515..339P 1703 T K A D     X C F     38 18 2 First optical identification of the SRG/eROSITA-detected supernova remnant
G 116.6 - 26.1. I. Preliminary results.
PALAIOLOGOU E.V., LEONIDAKI I. and KOPSACHEILI M.
2023MNRAS.521.5536K 392           X         9 31 1 SRG/eROSITA discovery of a radio-faint X-ray candidate supernova remnant SRGe J003602.3+605421 = G121.1-1.9. KHABIBULLIN I.I., CHURAZOV E.M., BYKOV A.M., et al.
2023ApJ...957...82F 44           X         1 29 ~ The Spatial and Emission Properties of the Large [O III] Emission Nebula Near M31. FESEN R.A., KIMESWENGER S., SHULL J.M., et al.
2024A&A...689A.278K 179           X C       3 7 ~ Study of X-ray emission from the S147 nebula by SRG/eROSITA: Supernova-in-the-cavity scenario. KHABIBULLIN I.I., CHURAZOV E.M., CHUGAI N.N., et al.
2025RAA....25i5001L 3294 T   A S   X C       68 8 ~ The FAST Detection of an H I Cloud around
Supernova Remnant

G116.6-26.1
.
LIANG T., WANG J., WANG T., et al.
2025A&A...701A..21D 187           X         4 6 ~ Supernova explosions of runaway stars and young neutron stars above the Galactic plane. DAKIC V., POPOV S.B. and TUROLLA R.
2025A&A...701A..43G 65       D     X         2 11 ~ Multi-wavelength study of the high Galactic latitude supernova remnant candidate G118.4+37.0 associated with the Calvera pulsar. GRECO E., RIGOSELLI M., MEREGHETTI S., et al.
2025ApJ...992L...6S 93             C       1 11 ~ Absence of Radio Emission Reveals an Exceptionally Weak Explosion of the Putative Historical Supernova Pa 30. SHAO Y.-X., ZHOU P., ZHANG X., et al.

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