Utilización de microhilos magnéticos para promover la muerte de células de osteosarcoma mediante hipertermia magnética in vitro

Los tratamientos para el cáncer que se llevan a cabo actualmente tienen una serie de limitaciones que, unido a que se trata de técnicas invasivas, hace que se tienda a buscar nuevas alternativas. Una de ellas es la hipertermia dirigida, cuyo objetivo son las células cancerígenas. Se trata de una técnica relativamente nueva, por lo que aún no se ha estudiado en profundidad. En este trabajo, se han utilizado microhilos magnéticos amorfos recubiertos de vidrio para calentar células de osteosarcoma aplicando un campo magnético alterno. De acuerdo con los resultados obtenidos de los ensayos realizados “in vitro”, se puede confirmar que la utilización de estos microhilos magnéticos reduce la proliferación de células cancerígenas dando lugar finalmente a la muerte celular. Además, esta técnica es un proceso mucho menos invasivo que los utilizados actualmente y que requiere exposiciones breves a campos magnéticos débiles. Por todo esto, la hipertermia dirigida se presenta como una alternativa efectiva para el tratamiento de osteosarcoma.Por último, agradecer a Tamag Ibérica S.L. por proporcionarnos los microhilos magnéticos para poder llevar a cabo este estudio y a Fomento de San Sebastián por financiar el proyecto de investigació

Utilización de microhilos magnéticos para promover la muerte de células de osteosarcoma mediante hipertermia magnética in vitro

Los tratamientos para el cáncer que se llevan a cabo actualmente tienen una serie de limitaciones que, unido a que se trata de técnicas invasivas, hace que se tienda a buscar nuevas alternativas. Una de ellas es la hipertermia dirigida, cuyo objetivo son las células cancerígenas. Se trata de una técnica relativamente nueva, por lo que aún no se ha estudiado en profundidad. En este trabajo, se han utilizado microhilos magnéticos amorfos recubiertos de vidrio para calentar células de osteosarcoma aplicando un campo magnético alterno. De acuerdo con los resultados obtenidos de los ensayos realizados “in vitro”, se puede confirmar que la utilización de estos microhilos magnéticos reduce la proliferación de células cancerígenas dando lugar finalmente a la muerte celular. Además, esta técnica es un proceso mucho menos invasivo que los utilizados actualmente y que requiere exposiciones breves a campos magnéticos débiles. Por todo esto, la hipertermia dirigida se presenta como una alternativa efectiva para el tratamiento de osteosarcoma.Por último, agradecer a Tamag Ibérica S.L. por proporcionarnos los microhilos magnéticos para poder llevar a cabo este estudio y a Fomento de San Sebastián por financiar el proyecto de investigació

J-PLUS: The javalambre photometric local universe survey

ABSTRACT: TheJavalambrePhotometric Local UniverseSurvey (J-PLUS )isanongoing 12-band photometricopticalsurvey, observingthousands of squaredegrees of theNorthernHemispherefromthededicated JAST/T80 telescope at the Observatorio Astrofísico de Javalambre (OAJ). The T80Cam is a camera with a field of view of 2 deg2 mountedon a telescopewith a diameter of 83 cm, and isequippedwith a uniquesystem of filtersspanningtheentireopticalrange (3500–10 000 Å). Thisfiltersystemis a combination of broad-, medium-, and narrow-band filters, optimallydesigned to extracttherest-framespectralfeatures (the 3700–4000 Å Balmer break region, Hδ, Ca H+K, the G band, and the Mg b and Ca triplets) that are key to characterizingstellartypes and delivering a low-resolutionphotospectrumforeach pixel of theobservedsky. With a typicaldepth of AB ∼21.25 mag per band, thisfilter set thusallowsforanunbiased and accuratecharacterization of thestellarpopulation in our Galaxy, itprovidesanunprecedented 2D photospectralinformationforall resolved galaxies in the local Universe, as well as accuratephoto-z estimates (at the δ z/(1 + z)∼0.005–0.03 precisionlevel) formoderatelybright (up to r ∼ 20 mag) extragalacticsources. Whilesomenarrow-band filters are designedforthestudy of particular emissionfeatures ([O II]/λ3727, Hα/λ6563) up to z < 0.017, theyalsoprovidewell-definedwindowsfortheanalysis of otheremissionlines at higherredshifts. As a result, J-PLUS has thepotential to contribute to a widerange of fields in Astrophysics, both in thenearbyUniverse (MilkyWaystructure, globular clusters, 2D IFU-likestudies, stellarpopulations of nearby and moderate-redshiftgalaxies, clusters of galaxies) and at highredshifts (emission-line galaxies at z ≈ 0.77, 2.2, and 4.4, quasi-stellarobjects, etc.). Withthispaper, wereleasethefirst∼1000 deg2 of J-PLUS data, containingabout 4.3 millionstars and 3.0 milliongalaxies at r <  21mag. With a goal of 8500 deg2 forthe total J-PLUS footprint, thesenumbers are expected to rise to about 35 millionstars and 24 milliongalaxiesbytheend of thesurvey.Funding for the J-PLUS Project has been provided by the Governments of Spain and Aragón through the Fondo de Inversiones de Teruel, the Spanish Ministry of Economy and Competitiveness (MINECO; under grants AYA2017-86274-P, AYA2016-77846-P, AYA2016-77237-C3-1-P, AYA2015-66211-C2-1-P, AYA2015-66211-C2-2, AYA2012-30789, AGAUR grant SGR-661/2017, and ICTS-2009-14), and European FEDER funding (FCDD10-4E-867, FCDD13-4E-2685

Glass-coated ferromagnetic microwire-induced magnetic hyperthermia for in vitro cancer cell treatment

Limitations in effectiveness and the invasive nature of current cancer treatment options emphasize the need for further clinical advancements. Among other approaches, targeted hyperthermia is as a new strategy aimed at targeting cancerous cells to improve the efficacy of radiotherapy or cytotoxic drugs. However, the testing of magnetic vehicles has mainly focused on the use of nanoparticles. In this work, Fe77B10Si10C3 glass-coated amorphous magnetic microwires were assessed for the first time as magnetic vehicles with high potential for the localized heating of osteosarcoma cells by means of an AC magnetic field. The results from the in vitro assays performed inside a microfluidic device demonstrated the ability of these magnetic microwires to induce malignant cell death. Exposing the system to different magnetic fields for less than 1 h provoked a reduction up to 89% of the osteosarcoma cell population, whereas healthy myoblastoma cells remained nearly unaffected. The proposed technology demonstrates in vitro the effectiveness of these microwires as vehicles for targeted magnetic hyperthermia

Utilización de microhilos magnéticos para promover la muerte de células de osteosarcoma mediante hipertermia magnética in vitro

Los tratamientos para el cáncer que se llevan a cabo actualmente tienen una serie de limitaciones que, unido a que se trata de técnicas invasivas, hace que se tienda a buscar nuevas alternativas. Una de ellas es la hipertermia dirigida, cuyo objetivo son las células cancerígenas. Se trata de una técnica relativamente nueva, por lo que aún no se ha estudiado en profundidad. En este trabajo, se han utilizado microhilos magnéticos amorfos recubiertos de vidrio para calentar células de osteosarcoma aplicando un campo magnético alterno. De acuerdo con los resultados obtenidos de los ensayos realizados “in vitro”, se puede confirmar que la utilización de estos microhilos magnéticos reduce la proliferación de células cancerígenas dando lugar finalmente a la muerte celular. Además, esta técnica es un proceso mucho menos invasivo que los utilizados actualmente y que requiere exposiciones breves a campos magnéticos débiles. Por todo esto, la hipertermia dirigida se presenta como una alternativa efectiva para el tratamiento de osteosarcoma.Por último, agradecer a Tamag Ibérica S.L. por proporcionarnos los microhilos magnéticos para poder llevar a cabo este estudio y a Fomento de San Sebastián por financiar el proyecto de investigació

Dust properties in H II regions in M 33

Context. The infrared emission (IR) of the interstellar dust has been claimed to be a tracer of the star formation rate. However, the conversion of the IR emission into star formation rate can be strongly dependent on the physical properties of the dust, which are affected by the environmental conditions where the dust is embedded. Aims: We study here the dust properties of a set of H ii regions in the Local Group galaxy M 33 presenting different spatial configurations between the stars, gas, and dust to understand the dust evolution in different environments. Methods: We modelled the spectral energy distribution (SED) of each region using the DustEM tool and obtained the mass relative to hydrogen for very small grains (VSG, YVSG), polycyclic aromatic hydrocarbons (YPAH), and big grains (BG, YBG). We furthermore performed a pixel-by-pixel SED modelling and derived maps of the relative mass of each grain type for the whole surface of the two most luminous H ii regions in M 33, NGC 604 and NGC 595. Results: The relative mass of the VSGs (YVSG/YTOTAL) changes with the morphology of the region: YVSG/YTOTAL is a factor of 1.7 higher for H ii regions classified as filled and mixed than for regions presenting a shell structure. The enhancement in VSGs within NGC 604 and NGC 595 is correlated to expansive gas structures with velocities ≥50 km s-1. The gas-to-dust ratio derived for the H ii regions in our sample exhibits two regimes related to the H i-H2 transition of the interstellar medium (ISM). Regions corresponding to the H i diffuse regime present a gas-to-dust ratio compatible with the expected value if we assume that the gas-to-dust ratio scales linearly with metallicity, while regions corresponding to a H2 molecular phase present a flatter dust-gas surface density distribution. Conclusions: The fraction of VSGs can be affected by the conditions of the interstellar environment: strong shocks of 50-90 km s-1 existing in the interior of the most luminous H ii regions can lead to fragmentation of BGs into smaller ones, while the more evolved shell and clear shell objects provide a more quiescent environment where reformation of dust BGs might occur. The gas-to-dust variations found in this analysis might imply that grain coagulation and/or gas-phase metal incorporation into the dust mass is occurring in the interior of the H ii regions in M 33.Full Tables A.1 and A.2 are only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/595/A4

Accounting and Business Economics in Spain

Economia de la Empresa (Business Economics) emerged in Spain as a distinct academic discipline in the second half of the twentieth century. In its early years, Business Economics shared common influences with Accounting, particularly ideas and theories acquired from the translation of Italian and German works on Economia Aziendale and Betriebswirtschaftslehre. However, partly because of the institutional structure of Spanish universities, the two disciplines moved apart. During the Franco regime, Spanish accounting research was quite isolated, and with the return of democracy and the move towards greater European involvement much research was devoted to issues of financial accounting harmonization and standardization. This normative research was of little interest to Business Economics researchers, who were developing analytical approaches grounded in economic theory. More recently, academics working in the two disciplines have drawn on a wider range of theoretical approaches, from empirical studies to behavioural and organizational theory and institutional economics based on agency theory and transaction cost analysis. At present, the disciplines 'walk separately down the same road', but the new generation of researchers has the opportunity to bring Accounting and Business Economics closer together from an intellectual and scientific point of view.