CARACTERIZAÇÃO MORFOMÉTRICA E MORFOLÓGICA DE CÉLULA ESPERMÁTICA DE CAPIVARA (Hydrochoerus hydrochaeris)

Spermatic cells were obtained from 50 slaughtered capybaras of 2 groups (G1 and G2) and then evaluated for morphological aspects at light microscopy and scanning and transmission electron microscopy. Spermatic cells were fixed with methanol (G1) or 10% neutral buffered formol saline (G2) on glass slides and then evaluated in regard to normal and abnormal morphology, as described by BLOM (1973). A total of 52,62% of those evaluated cells showed abnormal morphology distributed as major defects (28,20%) or minor defects (24,42%), grouped on head, tail or midpiece defects; those were confirmed with scanning electron microscopy. The mean length and width of spermatic cell head and midpiece, and tail length were characterized by morphometric evaluation, respectively, as (x ± sd) 6,85 + 0,81 µm and 4,00 + 2,53 µm, 6,97 + 2,53 µm and 1,53 + 0,27 µm and 44,20 + 8,03 µm. The evaluation of spermatic cells by transmission electron microscopy have shown extended head with condensed nuclear chromatin and extremely dense nucleus; the spermatic cells tail was similar to other mammals.Células espermáticas de capivara foram obtidas de epidídimos de 50 animais abatidos em matadouro e divididos em dois grupos distintos (G1 e G2) e avaliadas quanto à morfologia em microscopia de luz e microscopia eletrônica de transmissão e varredura. Células fixadas em lâminas de vidro com metanol (G1) e formol salino (G2) foram avaliadas para identificação de defeitos, classificados segundo BLOM (1973). Os achados do presente estudo demonstraram que 52,6% das células avaliadas apresentavam defeitos em sua morfologia, sendo estes distribuídos em defeitos maiores (28,20%) e menores (24,42%), e agrupados em defeitos de cabeça, cauda e peça intermediária. Os mesmos foram confirmados pela microscopia eletrônica de varredura. Através da avaliação morfométrica foi possível caracterizar o comprimento e a largura da cabeça e peça intermediária, e comprimento de cauda espermática (x ± sd) respectivamente, 6,85 + 0,81 µm e 4,00 + 2,53 µm, 6,97 + 2,53 µm e 1,53 + 0,27 µm e 44,20 + 8,03 µm. Pela microscopia eletrônica de transmissão caracterizou-se a cabeça espermática alongada, com cromatina nuclear condensada e núcleo extremamente denso; a cauda espermática demonstrou ser semelhante à de outros mamíferos

EUPRON: nurses’ practice in interprofessional pharmaceutical care in Europe. A cross-sectional survey in 17 countries

Abstract Objectives Safe pharmaceutical care (PC) requires an interprofessional team approach, involving physicians, nurses and pharmacists. Nurses’ roles however, are not always explicit and clear, complicating interprofessional collaboration. The aim of this study is to describe nurses’ practice and interprofessional collaboration in PC, from the viewpoint of nurses, physicians and pharmacists. Design A cross-sectional survey. Setting The study was conducted in 17 European countries, each with their own health systems. Participants Pharmacists, physicians and nurses with an active role in PC were surveyed. Main outcome measures Nurses’ involvement in PC, experiences of interprofessional collaboration and communication and views on nurses’ competences. Results A total of 4888 nurses, 974 physicians and 857 pharmacists from 17 European countries responded. Providing patient education and information (PEI), monitoring medicines adherence (MMA), monitoring adverse/therapeutic effects (ME) and prescribing medicines were considered integral to nursing practice by 78%, 73%, 69% and 15% of nurses, respectively. Most respondents were convinced that quality of PC would be improved by increasing nurses’ involvement in ME (95%), MMA (95%), PEI (91%) and prescribing (53%). Mean scores for the reported quality of collaboration between nurses and physicians, collaboration between nurses and pharmacists and interprofessional communication were respectively <7/10, ≤4/10, <6/10 for all four aspects of PC. Conclusions ME, MMA, PEI and prescribing are part of nurses’ activities, and most healthcare professionals felt their involvement should be extended. Collaboration between nurses and physicians on PC is limited and between nurses and pharmacists even more

The TESS-Keck Survey. II. An Ultra-Short-Period Rocky Planet And Its Siblings Transiting The Galactic Thick-Disk Star TOI-561

We report the discovery of TOI-561, a multiplanet system in the galactic thick disk that contains a rocky, ultra-short-period planet. This bright (V = 10.2) star hosts three small transiting planets identified in photometry from the NASA TESS mission: TOI-561 b (TOI-561.02, P = 0.44 days, Rp = 1.45 ± 0.11 R⊕), c (TOI-561.01, P = 10.8 days, Rp = 2.90 ± 0.13 R⊕), and d (TOI-561.03, P = 16.3 days, Rp = 2.32 ± 0.16 R⊕). The star is chemically ([Fe/H] = −0.41 ± 0.05, [α/Fe] = +0.23 ± 0.05) and kinematically consistent with the galactic thick-disk population, making TOI-561 one of the oldest (10 ± 3 Gyr) and most metal-poor planetary systems discovered yet. We dynamically confirm planets b and c with radial velocities from the W. M. Keck Observatory High Resolution Echelle Spectrometer. Planet b has a mass and density of 3.2 ± 0.8 M⊕ and ${5.5}_{-1.6}^{+2.0}$g cm−3, consistent with a rocky composition. Its lower-than-average density is consistent with an iron-poor composition, although an Earth-like iron-to-silicates ratio is not ruled out. Planet c is 7.0 ± 2.3 M⊕ and 1.6 ± 0.6 g cm−3, consistent with an interior rocky core overlaid with a low-mass volatile envelope. Several attributes of the photometry for planet d (which we did not detect dynamically) complicate the analysis, but we vet the planet with high-contrast imaging, ground-based photometric follow-up, and radial velocities. TOI-561 b is the first rocky world around a galactic thick-disk star confirmed with radial velocities and one of the best rocky planets for thermal emission studies

The NUPHAC-EU Framework for Nurses' Role in Interprofessional Pharmaceutical Care: Cross-Sectional Evaluation in Europe.

Clear role descriptions promote the quality of interprofessional collaboration. Currently, it is unclear to what extent healthcare professionals consider pharmaceutical care (PC) activities to be nurses' responsibility in order to obtain best care quality. This study aimed to create and evaluate a framework describing potential nursing tasks in PC and to investigate nurses' level of responsibility. A framework of PC tasks and contextual factors was developed based on literature review and previous DeMoPhaC project results. Tasks and context were cross-sectionally evaluated using an online survey in 14 European countries. A total of 923 nurses, 240 physicians and 199 pharmacists responded. The majority would consider nurses responsible for tasks within: medication self-management (86-97%), patient education (85-96%), medication safety (83-95%), monitoring adherence (82-97%), care coordination (82-95%), and drug monitoring (78-96%). The most prevalent level of responsibility was 'with shared responsibility'. Prescription management tasks were considered to be nurses' responsibility by 48-81% of the professionals. All contextual factors were indicated as being relevant for nurses' role in PC by at least 74% of the participants. No task nor contextual factor was removed from the framework after evaluation. This framework can be used to enable healthcare professionals to openly discuss allocation of specific (shared) responsibilities and tasks

The L 98-59 System: Three Transiting, Terrestrial-Size Planets Orbiting A Nearby M Dwarf

We report the Transiting Exoplanet Survey Satellite (TESS) discovery of three terrestrial-size planets transiting L 98-59 (TOI-175, TIC 307210830)—a bright M dwarf at a distance of 10.6 pc. Using the Gaia-measured distance and broadband photometry, we find that the host star is an M3 dwarf. Combined with the TESS transits from three sectors, the corresponding stellar parameters yield planet radii ranging from 0.8 R⊕ to 1.6 R⊕. All three planets have short orbital periods, ranging from 2.25 to 7.45 days with the outer pair just wide of a 2:1 period resonance. Diagnostic tests produced by the TESS Data Validation Report and the vetting package DAVE rule out common false-positive sources. These analyses, along with dedicated follow-up and the multiplicity of the system, lend confidence that the observed signals are caused by planets transiting L 98-59 and are not associated with other sources in the field. The L 98-59 system is interesting for a number of reasons: the host star is bright (V = 11.7 mag, K = 7.1 mag) and the planets are prime targets for further follow-up observations including precision radial-velocity mass measurements and future transit spectroscopy with the James Webb Space Telescope; the near-resonant configuration makes the system a laboratory to study planetary system dynamical evolution; and three planets of relatively similar size in the same system present an opportunity to study terrestrial planets where other variables (age, metallicity, etc.) can be held constant. L 98-59 will be observed in four more TESS sectors, which will provide a wealth of information on the three currently known planets and have the potential to reveal additional planets in the system

The TESS-keck survey. III. A stellar obliquity measurement of TOI-1726 c

We report the measurement of a spectroscopic transit of TOI-1726c, one of two planets transiting a G-type star with V = 6.9 in the Ursa Major Moving Group (∼400 Myr). With a precise age constraint from cluster membership, TOI-1726 provides a great opportunity to test various obliquity excitation scenarios that operate on different timescales. By modeling the Rossiter-McLaughlin (RM) effect, we derived a sky-projected obliquity of -1-+3235∘. This result rules out a polar/retrograde orbit and is consistent with an aligned orbit for planet c. Considering the previously reported, similarly prograde RM measurement of planet b and the transiting nature of both planets, TOI-1726 tentatively conforms to the overall picture that compact multitransiting planetary systems tend to have coplanar, likely aligned orbits. TOI-1726 is also a great atmospheric target for understanding differential atmospheric loss of sub-Neptune planets (planet b 2.2 R☉ and c 2.7 R☉ both likely underwent photoevaporation). The coplanar geometry points to a dynamically cold history of the system that simplifies any future modeling of atmospheric escape