SNR G330.2+01.0 (Spanish Wikipedia)

Analysis of information sources in references of the Wikipedia article "SNR G330.2+01.0" in Spanish language version.

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Williams, Brian J. et al. (2018). «A Deep X-Ray View of the Synchrotron-dominated Supernova Remnant G330.2+1.0». The Astrophysical Journal 855 (2): 9 pp. 118. Consultado el 7 de octubre de 2021.
Torii, Ken'ichi; Uchida, Hiroyuki; Hasuike, Kazuto; Tsunemi, Hiroshi; Yamaguchi, Yasuhiro; Shibata, Shinpei (2006). «Discovery of a Featureless X-Ray Spectrum in the Supernova Remnant Shell of G330.2+1.0». Publications of the Astronomical Society of Japan 58 (1): L11-L14. Consultado el 7 de octubre de 2021.
Borkowski, K.J. et al. (2018). «Expansion and Age of the X-Ray Synchrotron-dominated Supernova Remnant G330.2+1.0». The Astrophysical Journal Letters 868 (2): 5 pp. L21. Consultado el 7 de octubre de 2021.
Park, Sangwook; Kargaltsev, Oleg; Pavlov, George G.; Mori, Koji; Slane, Patrick O.; Hughes, John P.; Burrows, David N.; Garmire, Gordon P. (2009). «Nonthermal X-Rays from Supernova Remnant G330.2+1.0 and the Characteristics of its Central Compact Object». The Astrophysical Journal 695 (1): 431-441. Consultado el 7 de octubre de 2021.
Park, Sangwook et al. (2006). «Discovery of a Candidate Central Compact Object in the Galactic Nonthermal SNR G330.2+1.0». The Astrophysical Journal 653 (1): L37-L40. Consultado el 7 de octubre de 2021.

Clark, D.H. et al. (1975). «408 and 5000 mhz observations of 28 new galactic supernova remnants». Australian Journal of Physics 37: 1-38. Consultado el 7 de octubre de 2021.