34 research outputs found
Carcass physical composition and meat quality of holstein calves, terminated in different finishing systems and slaughter weights
Comparing Pedagogical Innovations
Innovation seems to be a constant – and necessary – theme in education. A common underlying rationale is that changes in education of all levels and types prepare citizens for life in the knowledge society. The contexts include intensifying globalisation, progressively shorter half-lives of knowledge, and economic competitiveness which requires increased collaboration and different ways of working (Hershock et al. 2007; Scardamalia & Bereiter 2010). As the creation and dissemination of knowledge are perceived to be of paramount importance, education requires new goals and processes. This view is applicable both in economically advanced countries (e.g. European Round Table of Industrialists 1997; OECD 2004) and in less developed countries (e.g. UNESCO 2003; Kozma 2008)
The novel BH3 α-helix mimetic JY-1-106 induces apoptosis in a subset of cancer cells (lung cancer, colon cancer and mesothelioma) by disrupting Bcl-xL and Mcl-1 protein–protein interactions with Bak
Time-synchronized immune-guided SBRT partial bulky tumor irradiation targeting hypoxic segment while sparing the peritumoral immune microenvironment
Mono-institutional phase 2 study of innovative Stereotactic Body RadioTherapy targeting PArtial Tumor HYpoxic (SBRT-PATHY) clonogenic cells in unresectable bulky non-small cell lung cancer: profound non-targeted effects by sparing peri-tumoral immune microenvironment
The complex gaseous and stellar environments of the nearby dual active galactic nucleus mrk 739
none10siWe present integral field spectroscopic observations of the nearby (z ∼ 0.03) dual active galactic nuclei (AGNs) Mrk 739, whose projected nuclear separation is ∼3.4 kpc, obtained with the Multi Unit Spectroscopic Explorer at the Very Large Telescope. We find that the galaxy has an extended AGN-ionized emission-line region extending up to ∼20 kpc away from the nuclei, while star-forming regions are more centrally concentrated within 2-3 kpc. We model the kinematics of the ionized gas surrounding the eastern nucleus using a circular disk profile, resulting in a peak velocity of - 237+ km s- 28 26 1 at a distance of ∼1.2 kpc. The enclosed dynamical mass within 1.2 kpc is logM(M⊙) = 10.20 ±0.06, ∼1000 times larger than the estimated supermassive black hole (SMBH) mass of Mrk 739E. The morphology and dynamics of the system are consistent with an early stage of the collision, where the foreground galaxy (Mrk 739W) is a young star-forming galaxy in an ongoing first passage with its background companion (Mrk 739E). Since the SMBH in Mrk 739W does not show evidence of being rapidly accreting, we claim that the northern spiral arms of Mrk 739W are ionized by the nuclear activity of Mrk 739E. © 2021 Institute of Physics Publishing. All rights reserved.openTubín, D.; Treister, E.; D'Ago, G.; Venturi, G.; Bauer, F.E.; Privon, G.C.; Koss, M.J.; Ricci, F.; Comerford, J.M.; Müller-Sánchez, F.Tubín, D.; Treister, E.; D'Ago, G.; Venturi, G.; Bauer, F.E.; Privon, G.C.; Koss, M.J.; Ricci, F.; Comerford, J.M.; Müller-Sánchez, F