Zobrazeno 1 - 10
of 236
pro vyhledávání: '"G. Migliori"'
Publikováno v:
Pulmonology, Vol 24, Iss 2, Pp 106-114 (2018)
Tuberculosis (TB) is a major cause of childhood morbidity and mortality worldwide. The aim of this review is to describe the management of the child with TB and latent tuberculosis infection (LTBI).To develop this article, a working group reviewed re
Externí odkaz:
https://doaj.org/article/0344660c42e24059962e20935bacced7
Publikováno v:
Italian Journal of Animal Science, Vol 2, Iss 1S, Pp 148-150 (2011)
Forty buffalo heifers of approximately 19 months of age were used. Subjects, with a mean live weight of 390 kg, were randomly and equally allocated for 12 weeks to 4 groups. Thus, the experimental design was a 2 x 2 factorial with two space allowance
Externí odkaz:
https://doaj.org/article/1c9432899fa94c5bb495cf7cc902575b
Publikováno v:
Italian Journal of Animal Science, Vol 4, Iss 2s, Pp 409-411 (2010)
Early experience is well known to strongly condition adult behavior and contact with humans is a determinant factor influencing behavioral and emotional characteristics of young animals. For horse husbandry a successful human-animal relationship is v
Externí odkaz:
https://doaj.org/article/8a8c5b6bf22b47fb810ce73d82c347d3
Autor:
G Migliori, A Siemiginowska, C C Cheung, A Celotti, M Giroletti, G Giovannini, A Paggi, E Liuzzo
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 512:4639-4659
We report the discovery of a bright, extended X-ray jet in the quasar RGB J1512+020A (z = 0.22). Chandra observations show the X-ray core and 13 arcsec (∼45 kpc projected) extended emission coincident with the radio jet. The jet stands out as one o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7d38e5b97f46001b32ca387408503da2
https://doi.org/10.1093/mnras/stac514
https://doi.org/10.1093/mnras/stac514
The incidence of young but fading radio sources provides important information on the life cycle of radio emission in radio-loud active galactic nuclei. Despite its importance for constraining the models of radio source evolution, there are no system
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c80832e513134d4683194609aca3be8
Autor:
M. Orienti, Giacomo Principe, F. D'Ammando, Mn Mazziotta, G. Migliori, L. Di Venere, Marcello Giroletti
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:4564-4583
According to radiative models, radio galaxies and quasars are predicted to produce gamma rays from the earliest stages of their evolution. Exploring their high-energy emission is crucial for providing information on the most energetic processes, the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0b40b25d46757534b03a1f7980739a65
https://doi.org/10.1093/mnras/stab2357
https://doi.org/10.1093/mnras/stab2357
Akademický článek
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Autor:
G. Migliori, B. De Marco, Vladimir Karas, P. G. Boorman, Bozena Czerny, Agata Różańska, T. P. Adhikari, A. Borkar, Alex Markowitz
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 500:3536-3551
We study the multi-phase medium in the vicinity of the active galactic nucleus Centaurus A (Cen A). Combined high-resolution observations with the ALMA and Chandra observatories indicate that the hot X-ray emitting plasma coexists with the warm and c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::55f32c7d766860151d89d9ac028b4f99
https://doi.org/10.1093/mnras/staa3515
https://doi.org/10.1093/mnras/staa3515
Publikováno v:
Astronomy & Astrophysics. 670:A35
We present the discovery and the subsequent follow up of radio emission from SDSS J130402.36$+$293840.6 (J1304+2938), the candidate host galaxy of the gamma-ray burst GRB~200716C. The galaxy is detected in the RACS (0.89 GHz), the NVSS, the Apertif i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::87204155ae3577e3d5fdd3509583666c
https://doi.org/10.1051/0004-6361/202243829
https://doi.org/10.1051/0004-6361/202243829
Akademický článek
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