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SNR G011.0+00.0 , the SIMBAD biblio (35 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST06:10:44 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
---|---|---|---|---|---|---|---|---|---|
2003ApJ...589..253B | 37 | K | 27 | 49 | Diffuse hard X-ray sources discovered with the ASCA galactic plane survey. | BAMBA A., UENO M., KOYAMA K., et al. | |||
2003AN....324...52E | 22 | 4 | Galactic X-ray surveys. | EBISAWA K., YAMAUCHI S., BAMBA A., et al. | |||||
2003AN....324..139B | 6 | 1 | Search for synchrotron X-ray dominated SNRs in the ASCA Galactic plane survey. | BAMBA A., UENO M., KOYAMA K., et al. | |||||
2004AJ....127..355B | 21 | 18 | A low-frequency survey of the galactic plane near l=11°: discovery of three new supernova remnants. | BROGAN C.L., DEVINE K.E., LAZIO T.J., et al. | |||||
2004PASJ...56.1059Y | 14 | 14 | XMM-Newton observations of G32.45+0.1 and G38.55+0.0: diffuse hard X-ray sources found by the ASCA Galactic Plane Survey. | YAMAGUCHI H., UENO M., KOYAMA K., et al. | |||||
2006A&A...450..569P | 2 | 42 | 216 | Ammonia in infrared dark clouds. | PILLAI T., WYROWSKI F., CAREY S.J., et al. | ||||
2006ApJ...639L..25B | 2 | 43 | 191 | Discovery of 35 new supernova remnants in the inner Galaxy. | BROGAN C.L., GELFAND J.D., GAENSLER B.M., et al. | ||||
2007A&A...472..489A | 151 | X C | 3 | 21 | 62 | Discovery of two candidate pulsar wind nebulae in very-high-energy gamma rays. | AHARONIAN F., AKHPERJANIAN A.G., BAZER-BACHI A.R., et al. | ||
2007ApJ...670..655K | 30 | 30 | X-ray emission from PSR J1809-1917 and its pulsar wind nebula, possibly associated with the TeV gamma-ray source HESS J1809-193. | KARGALTSEV O. and PAVLOV G.G. | |||||
2009BASI...37...45G | 15 | D | 1 | 282 | 336 | A revised Galactic supernova remnant catalogue. | GREEN D.A. | ||
2010ApJ...721.1492P | 38 | X | 1 | 43 | 19 | Non-thermal X-ray emission from the northwestern rim of the galactic supernova remnant G266.2-1.2 (RX J0852.0-4622). | PANNUTI T.G., ALLEN G.E., FILIPOVIC M.D., et al. | ||
2011A&A...536A..83S | 115 | X F | 2 | 68 | 67 | A Sino-German λ6 cm polarization survey of the Galactic plane. VII. Small supernova remnants. | SUN X.H., REICH P., REICH W., et al. | ||
2013ApJS..204....4P | 16 | D | 1 | 232 | 37 | The radio surface-brightness-to-diameter relation for Galactic supernova remnants: sample selection and robust analysis with various fitting offsets. | PAVLOVIC M.Z., UROSEVIC D., VUKOTIC B., et al. | ||
2014BASI...42...47G | 16 | D | 1 | 294 | 240 | A catalogue of 294 Galactic supernova remnants. | GREEN D.A. | ||
2016A&A...587A..71C | 987 | A | O X C | 24 | 25 | 4 | Unveiling the origin of HESS J1809-193. | CASTELLETTI G., GIACANI E. and PETRIELLA A. | |
2016ApJS..224....8A | 16 | D | 1 | 300 | 196 | The first Fermi LAT supernova remnant catalog. | ACERO F., ACKERMANN M., AJELLO M., et al. | ||
2016MNRAS.458.3411T | 16 | D | 1 | 308 | 6 | Galactic survey of 44Ti sources with the IBIS telescope onboard INTEGRAL. | TSYGANKOV S.S., KRIVONOS R.A., LUTOVINOV A.A., et al. | ||
2017ApJ...843...40A | 42 | X | 1 | 134 | 227 | The 2HWC HAWC Observatory gamma-ray catalog. | ABEYSEKARA A.U., ALBERT A., ALFARO R., et al. | ||
2018ApJ...859...69A | 412 | X C | 9 | 34 | 4 | GeV emission in the region of HESS J1809-193 and HESS J1813-178 is HESS J1809-193 a proton pevatron? | ARAYA M. | ||
2018A&A...612A...1H | 1 | 186 | 227 | The H.E.S.S. Galactic plane survey. | HESS COLLABORATION, ABDALLA H., ABRAMOWSKI A., et al. | ||||
2018ApJ...867...61Z | 82 | C | 1 | 126 | 2 | How does the stellar wind influence the radio morphology of a supernova remnant? | ZHANG M.F., TIAN W.W. and WU D. | ||
2018ApJS..238...35S | 16 | D | 1 | 52 | 27 | Distances of galactic supernova remnants using red clump stars. | SHAN S.S., ZHU H., TIAN W.W., et al. | ||
2018ApJ...868..119K | 247 | X C | 5 | 16 | ~ | The variable pulsar wind nebula of PSR J1809-1917. | KLINGLER N., KARGALTSEV O., PAVLOV G.G., et al. | ||
2019AJ....157..123L | 17 | D | 1 | 97 | ~ | Near-infrared [Fe II] and H2 emission-line study of Galactic supernova remnants in the first quadrant. | LEE Y.-H., KOO B.-C., LEE J.-J., et al. | ||
2019JApA...40...36G | 17 | D | 1 | 294 | 163 | A revised catalogue of 294 Galactic supernova remnants. | GREEN D.A. | ||
2020MNRAS.493.2706C | 102 | D | C | 2 | 217 | 14 | A complete catalogue of dusty supernova remnants in the Galactic plane. | CHAWNER H., GOMEZ H.L., MATSUURA M., et al. | |
2020MNRAS.493.3159G | 17 | D | 1 | 116 | 25 | Realistic modelling of wind and supernovae shocks in star clusters: addressing 22Ne/20Ne and other problems in Galactic cosmic rays. | GUPTA S., NATH B.B., SHARMA P., et al. | ||
2020MNRAS.498.3736D | 639 | X | 15 | 9 | ~ | A magnetar parallax. | DING H., DELLER A.T., LOWER M.E., et al. | ||
2021ApJS..253...17S | 104 | D | C | 2 | 64 | 3 | Atlas of CO-line shells and cavities around Galactic supernova remnants with FUGIN. | SOFUE Y., KOHNO M. and UMEMOTO T. | |
2021A&A...651A..86D | 17 | D | 1 | 254 | 16 | A global view on star formation: The GLOSTAR Galactic plane survey. II. Supernova remnants in the first quadrant of the Milky Way. | DOKARA R., BRUNTHALER A., MENTEN K.M., et al. | ||
2022ApJ...940...63R | 18 | D | 1 | 224 | 8 | Distances, Radial Distribution, and Total Number of Galactic Supernova Remnants. | RANASINGHE S. and LEAHY D. | ||
2023A&A...672A.103H | 467 | X C | 9 | 15 | 2 | HESS J1809-193: A halo of escaped electrons around a pulsar wind nebula? | HESS COLLABORATION, AHARONIAN F., AIT BENKHALI F., et al. | ||
2023ApJ...949...90L | 233 | X C | 4 | 13 | ~ | Revisiting the Chandra Observation on the Region of PSR J1J1809-193: Indication of the Existence of an X-Ray Halo and Implication for the Origin of HESS J1809-193. | LI C.-M., GE C. and LIU R.-Y. | ||
2023ApJS..268...61Z | 65 | D | X | 2 | 249 | ~ | A Systematic Study of Associations between Supernova Remnants and Molecular Clouds. | ZHOU X., SU Y., YANG J., et al. | |
2024ApJ...961...61B | 680 | A | X C | 13 | 6 | ~ | HESS J1809-193: Gamma-Ray Emission by Cosmic Rays from a Past Explosion. | BOXI S. and GUPTA N. |