Search results for "NEB"

showing 10 items of 543 documents

Gamma-Ray Flares from Mrk421 in 2008 observed with the ARGO-YBJ detector

2010

In 2008 the blazar Markarian 421 entered a very active phase and was one of the brightest sources in the sky at TeV energies, showing frequent flaring episodes. Using the data of ARGO-YBJ, a full coverage air shower detector located at Yangbajing (4300 m a.s.l., Tibet, China), we monitored the source at gamma ray energies E > 0.3 TeV during the whole year. The observed flux was variable, with the strongest flares in March and June, in correlation with X-ray enhanced activity. While during specific episodes the TeV flux could be several times larger than the Crab Nebula one, the average emission from day 41 to 180 was almost twice the Crab level, with an integral flux of (3.6 +-0.6) 10^-1…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsBL Lacertae objectSettore FIS/05 - Astronomia E AstrofisicaExtended Air showersSettore FIS/05 - Astronomia e Astrofisicageneral" ["gamma rays]BlazarBL Lacertae objects; Markarian 421; gamma rays; Extended Air showersCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpectral indexindividual (Markarian 421)" ["BL Lacertae objects]Markarian 421Settore FIS/01 - Fisica SperimentaleGamma rayindividual (Markarian 421) - gamma rays: observations [BL Lacertae objects]Astronomy and AstrophysicsAir showerCrab NebulaSpace and Planetary Sciencegamma rayIntergalactic travelAstrophysics - High Energy Astrophysical Phenomena
researchProduct

Observation of TeV gamma rays from the Cygnus region with the ARGO-YBJ experiment

2012

We report the observation of TeV gamma-rays from the Cygnus region using the ARGO-YBJ data collected from 2007 November to 2011 August. Several TeV sources are located in this region including the two bright extended MGRO J2019+37 and MGRO J2031+41. According to the Milagro data set, at 20 TeV MGRO J2019+37 is the most significant source apart from the Crab Nebula. No signal from MGRO J2019+37 is detected by the ARGO-YBJ experiment, and the derived flux upper limits at 90% confidence level for all the events above 600 GeV with medium energy of 3 TeV are lower than the Milagro flux, implying that the source might be variable and hard to be identified as a pulsar wind nebula. The only statist…

Astrophysics::High Energy Astrophysical Phenomenageneral – pulsars: individual (MGRO J2019+37 [Gamma rays]FluxFOS: Physical sciencesAstrophysics01 natural sciencesPulsar wind nebulageneral – pulsar0103 physical sciencesMILAGRO010303 astronomy & astrophysicsDETECTORArgoPhysicsCALIBRATIONHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsMGRO J2031+41)Settore FIS/01 - Fisica SperimentaleGamma rayAstronomy and Astrophysicsindividual (MGRO J2019+37 MGRO J2031+41)PLANE3. Good healthMedium energyCrab Nebulagamma ray13. Climate actionSpace and Planetary ScienceGALACTIC SOURCESJ2032+4130Milagrogamma rays; general – pulsars; individual (MGRO J2019+37 MGRO J2031+41)EMISSIONAstrophysics - High Energy Astrophysical Phenomena
researchProduct

A study of the B and Be star population in the field of the LMC open cluster NGC 2004 with VLT-FLAMES

2005

Observations of hot stars belonging to the young cluster LMC-NGC2004 and its surrounding region have been obtained with the VLT-GIRAFFE facilities in MEDUSA mode. 25 Be stars were discovered; the proportion of Be stars compared to B-type stars is found to be of the same order in the LMC and in the Galaxy fields. 23 hot stars were discovered as spectroscopic binaries (SB1 and SB2), 5 of these are found to be eclipsing systems from the MACHO database, with periods of a few days. About 75% of the spectra in our sample are polluted by hydrogen (Halpha and Hgamma), [SII] and [NII] nebular lines. These lines are typical of HII regions. They could be associated with patchy nebulosities with a bi-m…

Be starPopulationFOS: Physical sciencesAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA01 natural sciencesbinaries: eclipsing [Stars]Spectral lineStars: early-type[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]ISM: nebular lines and bandsMagellanic Clouds [Galaxies]early-type [Stars]Stars: binaries: spectroscopic0103 physical sciencesCluster (physics)education010303 astronomy & astrophysicsStars: binaries: eclipsingPhysicseducation.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsStars: emission-lineAstrophysics (astro-ph)Stars: early-type ; Stars: emission-line Be ; Galaxies: Magellanic Clouds ; Stars: binaries: spectroscopic ; Stars: binaries: eclipsing ; ISM: lines and bandsAstronomy and AstrophysicsBeGalaxies: Magellanic CloudsGalaxyRadial velocityStarsbinaries: spectroscopic [Stars]Space and Planetary Scienceemission-line Be [Stars][SDU]Sciences of the Universe [physics]lines and bands [ISM]:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Open cluster
researchProduct

Inhalation solutions: which one are allowed to be mixed? Physico-chemical compatibility of drug solutions in nebulizers.

2006

AbstractTherapy of chronic respiratory diseases often involves inhalation therapy with nebulizers. Patients often attempt to shorten the time consuming administration procedure by mixing drug solutions/suspensions for simultaneous inhalation. This article considers the issue of physico-chemical compatibility of admixtures of drug solutions/suspensions in nebulizers.A search of databases, prescribing information and primary literature was conducted to locate literature concerning the physico-chemical compatibility of inhalation solutions/suspensions. This was supplemented by telephone interviews.Admixtures of albuterol with ipratropium and/or cromolyn, of albuterol and budesonide, or tobramy…

BudesonideDrugPulmonary and Respiratory MedicineRespiratory TherapyCystic Fibrosismedia_common.quotation_subjectReviewCompatibilityBenzalkonium chlorideAdministration InhalationCromolyn SodiummedicineDeoxyribonuclease IHumansAlbuterolPediatrics Perinatology and Child HealthAnti-Asthmatic AgentsBudesonideFenoterolmedia_commonExpectorantsInhalationbusiness.industryColistinIpratropiumNebulizers and VaporizersNebulizerAsthmaAcetylcysteineAnti-Bacterial AgentsBronchodilator AgentsNebulizerInhalation solutionsAnesthesiaPediatrics Perinatology and Child HealthIpratropiumColistinTobramycinDrug Therapy Combinationbusinessmedicine.drugJournal of cystic fibrosis : official journal of the European Cystic Fibrosis Society
researchProduct

ALMA spectral survey of Supernova 1987A – molecular inventory, chemistry, dynamics and explosive nucleosynthesis

2017

We report the first molecular line survey of Supernova 1987A in the millimetre wavelength range. In the ALMA 210--300 and 340--360 GHz spectra, we detected cold (20--170 K) CO, 28SiO, HCO+ and SO, with weaker lines of 29SiO from ejecta. This is the first identification of HCO+ and SO in a young supernova remnant. We find a dip in the J=6--5 and 5--4 SiO line profiles, suggesting that the ejecta morphology is likely elongated. The difference of the CO and SiO line profiles is consistent with hydrodynamic simulations, which show that Rayleigh-Taylor instabilities cause mixing of gas, with heavier elements much more disturbed, making more elongated structure. We obtained isotopologue ratios of…

CIRCUMSTELLAR RINGMetallicityLINE EMISSIONINFRARED WATER-VAPORFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energySpectral lineISM [radio lines]CORE-COLLAPSE SUPERNOVAENucleosynthesis0103 physical sciencesIsotopologueEjectaSupernova remnantLarge Magellanic CloudCARBON-MONOXIDE010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)molecules [ISM]QBHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsabundances [ISM]010308 nuclear & particles physicssupernova remnants [ISM]II-P SUPERNOVAEAstronomyindividual: Supernova 1987A [supernovae]NEBULA M 1-92Astronomy and AstrophysicsSupernovaAstrophysics - Solar and Stellar AstrophysicsPhysics and Astronomy13. Climate actionSpace and Planetary ScienceLARGE-MAGELLANIC-CLOUDAstrophysics - High Energy Astrophysical PhenomenaMASSIVE STARSSN 1987AMonthly Notices of the Royal Astronomical Society
researchProduct

Iekšējā kontrole nebanku kredītiestāde

2021

Diplomdarba tēma ir „Iekšējā kontrole nebanku kredītiestāde”. Pētījuma tēmas aktualitāte: uzņēmums X Rīgas filiāle darbojas finanšu produktu jomā, nav banka, bet izsniedz ātros kredītus, ir jānoskaidro trūkumi iekšējā vidē. Pētījuma objekts – uzņēmuma X Rīgas filiāles iekšējā kontrole. Pētījuma priekšmets – iekšējās kontroles elementi. Pētījuma tēmas aktualitāte: uzņēmuma X Rīgas filiālei, kura nav banka un darbojas finanšu produktu jomā, ir jānoskaidro trūkumi iekšējā vidē. Darbā tika izmantotā COSO modeļa pielietojums, kas parādīja, ka iekšējās kontroles sistēma kopumā atbilst COSO elementiem. Risku novērtēšanā ir daudz nepilnības. Uzņēmuma X Rīgas filiālei ir ieteicams vēl viens iekšējās…

COSOiekšējā kontroles sistēmanebanku kredītiestādesEkonomika un uzņēmējdarbībaātro kredītu devējs uzņēmums Xnebanku kontrole
researchProduct

Oratio Ioannis Baptistae Adrianii Habita Florentiae in sacris funebribus Caroli V Caesaris Augusti.

1562

Sign.: A8 Port. arquitectònica amb grav. xil.

Carles V emperador romanogermànic 1500-1558Carles I Rei d'Espanya (1500-1558)Oracions fúnebresOracions fúnebres
researchProduct

Oracion funebre en las ... exequias : que con assistencia de la ... Comunidad de los RR.PP. Agustinos ... celebraron en la iglesia parroquial del Sr.…

Esc. dels jesuïtes en fris p. 1 Fris, caplletres ornades, filets Grav. calc. amb retrat d'Antonia Carrovèr de San Agustin Text a 1 col. - Postil·les. - Reclams Sign.: ¶4, ¶¶4, ¶¶¶4, A-C4, D5

Carrover de San Agustín Antonia Oracions fúnebres Obres anteriors al 1800Sermons castellans S.XVIII Obres anteriors al 1800
researchProduct

Funebre memoria de la buena vida, muerte, y exequias del V. P. ... Fr. Jayme Castelló ... del Convento de la Virgen del Remedio de Valencia, del Ord…

1707

El f. de làm. és el retrat de Fr. Jaime Castelló Port. amb orla tip. Caplletres ornades, fris Sign.: [estrella]-2[estrella]4, A-E4, F2 Text amb postil·les marginals Reclams

Castelló Jaime (O.SS.T.) Exèquies Obres anteriors a 1800Oracions fúnebres València (Comunitat Valenciana) 1707 Obres anteriors a 1800
researchProduct

A rare case of sepsis due to Corynebacterium macginleyi from central venous catheter in an elderly woman

2011

Corynebacterium macginleyi is a gram positive rod that causes especially ocular infections: since now only six elderly cases of extraocular infection are described. A 76 years old bedridden woman with a central venous catheter was hospitalized for 10 days of persistent fever. She was treated before with vancomicin and then with imipenem. The clinical conditions improved and the patient was discharged after two weeks of hospitalization. Among recognised risk factors for this infection the advanced age, indwelling devices and immunosuppression seem the most important. On the other hand, the antibiotics of choice are glycopeptides while the association of another antibiotic is recommended in o…

Catheterization Central VenousTreatment OutcomeBacterial ProteinsCorynebacterium InfectionsRNA Ribosomal 16SSepsisHumansCorynebacterium macginleyi Sepsis Elderly ImmunosuppressionFemaleCorynebacteriumAgedAnti-Bacterial Agents
researchProduct