2009
DOI: 10.1016/j.geomorph.2009.03.026
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Bajada del Diablo impact crater-strewn field: The largest crater field in the Southern Hemisphere

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Cited by 19 publications
(21 citation statements)
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“…Reduced relicts of these flows, much more extended in past times, may be observed toward NW of the Filu-Có Meseta, where the G, D, D′, #26, #29, and #30 craters have been found, among many other craters of smaller size as indicated in Fig. 3 of Acevedo et al (2009). The observations performed in the exposed sections of the Puesto Marraco site identified a stratified sequence with occasional cut-and-fill structures, in which several layers are essentially interbedded ( Fig.…”
Section: The Origin and Characteristics Of The Pampa Sastre Formationmentioning
confidence: 83%
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“…Reduced relicts of these flows, much more extended in past times, may be observed toward NW of the Filu-Có Meseta, where the G, D, D′, #26, #29, and #30 craters have been found, among many other craters of smaller size as indicated in Fig. 3 of Acevedo et al (2009). The observations performed in the exposed sections of the Puesto Marraco site identified a stratified sequence with occasional cut-and-fill structures, in which several layers are essentially interbedded ( Fig.…”
Section: The Origin and Characteristics Of The Pampa Sastre Formationmentioning
confidence: 83%
“…The oldest rocks in the region are limestones and shales of the Santa Anita Formation (CallovianOxfordian). The Araucanian movements of the Andean Cordillera Cycle increased the relief through fault reactivation and overdeepening of the basins that controlled the sedimentation of continental epiclastic/ pyroclastic rocks (the Chubut Group, Albian-Turonian; Ardolino and Franchi, 1996;Acevedo et al, 2009).…”
Section: Geological Settingmentioning
confidence: 99%
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