Results 21 to 30 of about 893,592 (201)

La cerámica de Coscopunta, un sitio del Periodo Intermedio Tardío en la provincia de Carhuaz, Callejón de Huaylas, Perú

open access: yesBulletin de l'Institut Français d'Études Andines, 2015
This essay describes a large group of complete or nearly complete Late Intermediate Period pottery vessels uncovered by a farmer in 1979 at the site of Coscopunta, near the town of the Anta, Carhuaz Province, Ancash.
Richard L. Burger, Lucy C. Salazar
doaj   +1 more source

Un modelo etnográfico para interpretar el estilo técnico cerámico del Intermedio tardío (ap. 1100-1450 d. C.) en el altiplano de Carangas, Bolivia

open access: yesBulletin de l'Institut Français d'Études Andines, 2020
This text discusses the notion of pottery as a symbol for ethnic identity. This is crucial for the interpretative model of Señoríos Aymaras, which is widely accepted by pre-colonial archeology for the Late Intermediate Period (1100-1450 AD) in the ...
Juan Villanueva Criales
doaj   +1 more source

Obsidian in the Late-Inka Period of Antofagasta de la Sierra (Southern Argentinean Puna): basin bottom versus intermediate sectors? [PDF]

open access: yes, 2016
Este trabajo pretende aportar información acerca de la circulación de distintas variedades de obsidiana en la microrregión de Antofagasta de la Sierra con el objetivo de comenzar a evaluar algunas propuestas sobre aspectos de la organización político ...
Cohen, Maria Lorena   +2 more
core   +2 more sources

Armatambo y la sociedad Ychsma

open access: yesBulletin de l'Institut Français d'Études Andines, 2004
This document tries to describe in a provisional way the Ychsma cultural occupation of Armatambo archaeological site (south of Lima, Peru), during the Late Intermediate and Inca Periods.
Luisa E. Díaz Arriola
doaj   +1 more source

SN2012ab: A Peculiar Type IIn Supernova with Aspherical Circumstellar Material [PDF]

open access: yes, 2017
We present photometry, spectra, and spectropolarimetry of supernova (SN) 2012ab, mostly obtained over the course of $\sim 300$ days after discovery.
Akerlof, Carl   +20 more
core   +3 more sources

OSTEOFITOSIS VERTEBRAL EN POBLACIONES PREHISPÁNICAS DE SAN PEDRO DE ATACAMA, NORTE DE CHILE

open access: yesEstudios Atacameños
Se estudió la osteofitosis vertebral como indicador de estrés físico en grupos humanos prehistóricos de San Pedro de Atacama, durante los períodos Medio (400 DC - 1000 DC) e Intermedio Tardío (1000 DC - 1450 DC).
Rocío López-Barrales   +4 more
doaj   +1 more source

X-ray and optical observations of 1RXS J154814.5-452845: a new intermediate polar with soft X-ray emission

open access: yes, 2002
We report the identification of the ROSAT all-sky survey source 1RXS J154814.5-452845as new intermediate polar and present the results from follow-up optical and X-ray observations.
Haberl, F., Motch, C., Zickgraf, F. -J.
core   +1 more source

Life in the late Intermediate Period at Armatambo, Peru [PDF]

open access: yes, 2018
Title from PDF of title page (University of Missouri--Columbia, viewed on October 18, 2012). ; The entire thesis text is included in the research.pdf file; the official abstract appears in the short.pdf file; a non-technical public abstract appears in the public.pdf file. ; Dissertation advisors: Dr. Robert A. Benfer and Dr. Deborah M. Pearsall ; Vita.
openaire   +2 more sources

Del Horizonte Medio al Horizonte Tardío en la costa sur central: el caso del valle de Asia

open access: yesBulletin de l'Institut Français d'Études Andines, 2004
The Asia valley, which is situated 100 km south of Lima, played an important role during the Middle Horizon. In fact, the funerary contexts of the Huaca Malena, as well as the elaborate textiles that were found in them, suggest a strong relationship with
Rommel Angeles Falcón   +1 more
doaj   +1 more source

The rotation and Galactic kinematics of mid M dwarfs in the Solar Neighborhood

open access: yes, 2015
Rotation is a directly-observable stellar property, and drives magnetic field generation and activity through a magnetic dynamo. Main sequence stars with masses below approximately 0.35Msun (mid-to-late M dwarfs) are fully-convective, and are expected to
Berta-Thompson, Zachory K.   +5 more
core   +1 more source

Home - About - Disclaimer - Privacy