ABSTRACT The present study aimed to determine the unique values of the entrepreneurial potential of clinical veterinarians and to evaluate this potential by using a reliable and valid measurement tool. The study material was the data obtained from a survey conducted between May 2020 and April 2021 that included 343 veterinarians who were actively working in a veterinarian clinic/outpatient clinic. The Turkish version of the Entrepreneurial Potential Assessment Inventory was used to collect the data. On the basis of the results of the explanatory factor analysis, confirmatory factor analysis, and improvement (modification) indices calculated from the survey data, a 7-factor structure was obtained. According to the results of the entrepreneurial potential scale for clinical veterinarians, the following sub-dimensions of the scale were listed according to their contribution to the total variance explained: “effective communicative leadership,” “strategic resource development,” “self-efficacy,” “innovative creativity,” “resilience-strength,” “motivation for economic freedom,” and “risk-taking propensity.” This ranking reveals a tendency to possess these characteristics in Türkiye for entrepreneurship potential regardless of the profession. In light of the obtained data, it is recommended to provide clinical veterinarians with training on the topics of forming social networks, taking responsibility, and developing emotional intelligence, which is not included in the scale, as well as to instigate the desire to become independent and economically motivated to improve their entrepreneurial potential. tool 202 34 clinicoutpatient clinic outpatient analysis modification (modification 7factor 7 subdimensions sub dimensions explained effective leadership, leadership strategic development, development selfefficacy, selfefficacy self efficacy, efficacy “self-efficacy, innovative creativity, creativity resiliencestrength, resiliencestrength resilience strength, strength “resilience-strength, motivation freedom, freedom risktaking risk propensity. propensity profession networks responsibility intelligence 20 3 “self-efficacy “resilience-strength 2

RESUMO O presente estudo teve como objetivo determinar os valores exclusivos do potencial empreendedor dos veterinários clínicos e avaliar esse potencial usando uma ferramenta de medição confiável e válida. O material do estudo foram os dados obtidos em uma pesquisa realizada entre maio de 2020 e abril de 2021, que incluiu 343 veterinários que trabalhavam ativamente em uma clínica veterinária/ambulatório. A versão turca do Inventário de Avaliação do Potencial Empreendedor foi usada para coletar os dados. Com base nos resultados da análise fatorial explicativa, da análise fatorial confirmatória e dos índices de melhoria (modificação) calculados a partir dos dados da pesquisa, foi obtida uma estrutura de sete fatores. De acordo com os resultados da escala de potencial empreendedor para veterinários clínicos, as seguintes subdimensões da escala foram listadas de acordo com sua contribuição para a variância total explicada: "liderança comunicativa eficaz", "desenvolvimento de recursos estratégicos", "autoeficácia", "criatividade inovadora", "resiliência-força", "motivação para liberdade econômica" e "propensão a assumir riscos". Essa classificação revela uma tendência a possuir essas características na Turquia para o potencial de empreendedorismo, independentemente da profissão. À luz dos dados obtidos, recomenda-se que os veterinários clínicos recebam treinamento sobre os tópicos de formação de redes sociais, assunção de responsabilidade e desenvolvimento de inteligência emocional, que não estão incluídos na escala, bem como instigar o desejo de se tornarem independentes e economicamente motivados para melhorar seu potencial empreendedor. válida 202 2021 34 veterináriaambulatório veterinária ambulatório veterinária/ambulatório explicativa modificação (modificação fatores explicada liderança eficaz, eficaz , eficaz" estratégicos, estratégicos estratégicos" autoeficácia, autoeficácia "autoeficácia" criatividade inovadora, inovadora inovadora" resiliênciaforça, resiliênciaforça resiliência força "resiliência-força" motivação econômica propensão riscos. riscos . riscos" empreendedorismo profissão recomendase recomenda sociais emocional 20 3 "autoeficácia "resiliência-força 2

Abstract Objectives This analysis describes the protocol of a study with a case-cohort to design to prospectively evaluate the incidence of subclinical atherosclerosis and Cardiovascular Disease (CVD) in Chronic Inflammatory Disease (CID) participants compared to non-diseased ones. Methods A high-risk group for CID was defined based on data collected in all visits on self-reported medical diagnosis, use of medicines, and levels of high-sensitivity C-Reactive Protein >10 mg/L. The comparison group is the Aleatory Cohort Sample (ACS): a group with 10% of participants selected at baseline who represent the entire cohort. In both groups, specific biomarkers for DIC, markers of subclinical atherosclerosis, and CVD morbimortality will be tested using weighted Cox. Results The high-risk group (n = 2,949; aged 53.6 ± 9.2; 65.5% women) and the ACS (n=1543; 52.2±8.8; 54.1% women) were identified. Beyond being older and mostly women, participants in the high-risk group present low average income (29.1% vs. 24.8%, p < 0.0001), higher BMI (Kg/m2) (28.1 vs. 26.9, p < 0.0001), higher waist circumference (cm) (93.3 vs. 91, p < 0.0001), higher frequencies of hypertension (40.2% vs. 34.5%, p < 0.0001), diabetes (20.7% vs. 17%, p = 0.003) depression (5.8% vs. 3.9%, p = 0.007) and higher levels of GlycA a new inflammatory marker (p < 0.0001) compared to the ACS. Conclusions The high-risk group selected mostly women, older, lower-income/education, higher BMI, waist circumference, and of hypertension, diabetes, depression, and higher levels of GlycA when compared to the ACS. The strategy chosen to define the high-risk group seems adequate given that multiple sociodemographic and clinical characteristics are compatible with CID.

We present the multi-color, five-year light curves and the radial velocities of the near-contact binary system KR Cyg. We derived the masses of the components as 2.88 ± 0.20 MΘ and 1.26 ± 0.07 MΘ and the radii as 2.59 ± 0.06 RΘ and 1.80 ± 0.04 RΘ. We also searched for the empirical determination of albedo and effective temperature of the cooler, less massive star of KRCyg, and of two similar near contact binaries AK CMi, and DO Cas. The residuals between the observed and computed fluxes are attributed to the effect of mutual illumination which heats the surface layers of the illuminated star and does vary not only its bolometric albedo but also its limb-darkening coefficient and gravity-brightening exponent. The effective albedos are generally smaller than that expected from an envelope of convective star. These results are preliminary and speculative.

Presentamos curvas de luz en varios colores y velocidades radiales obtenidas a lo largo de cinco años para la binaria en cuasi-contacto KR Cyg. Obtenemos para las masas de las componentes 2.88 ± 0.20 MΘ y 1.26 ± 0.07 MΘ, y para los radios 2.59 ±0.06 RΘ y 1.80 ±0.04 RΘ. También investigamos las determinaciones empíricas del albedo y la temperatura efectiva de la estrella más fría y menos masiva de KR Cyg, y de otras dos binarias en cuasi-contacto similares, AK CMi y DO Cas. Los residuos entre los flujos observados y los calculados se atribuyen al efecto de la iluminación mutua, la cual calienta las capas superficiales de la estrella iluminada y hace que varíe no sólo el albedo bolométrico, sino también el coeficiente del ennegrecimiento al limbo y el exponente del abrillantamiento por gravedad. Los albedos efectivos son generalmente menores que los esperados para la envolvente de una estrella convectiva. Nuestros resultados son preliminares y especulativos.

BVR light curves and radial velocities for the double-lined eclipsing binary V1135 Her were obtained. Our analyses of the multi-color light curves and radial velocities led to the determination of fundamental stellar properties of both components of the interesting system V1135 Her. The system consists of two evolved stars, G1+K3 between giants and supergiants, with masses of M1 = 1.461 ±0.054 M☉ and M2 = 0.504 ± 0.040 M☉ and radii of R1 = 27.1 ± 0.4 R☉ and R2 = 10.4 ± 0.2 R☉. Most of the observed and calculated parameters of the VI135 Her and its location on the color-magnitude and period-luminosity diagrams lead to a classification of an Anomalous Cepheid.

Se obtuvieron curvas de luz en BVR y velocidades radiales para la binaria eclipsante de doble línea V1135 Her. Nuestro análisis de las curvas de luz en varios colores y de las velocidades radiales nos permitió la determinación de propiedades estelares fundamentales para ambas componentes de este interesante sistema. El sistema está formado por dos estrellas evolucionadas G1+K3, intermedias entre gigantes y supergigantes, con masas M1= 1.461±0.054 M☉, M2 = 0.504±0.040 M☉, y radios R1 = 27.1 ±0.4 R☉, R2 = 10.4±0.2 R☉. La mayor parte de los parámetros observados y calculados para V1135 Her, así como su ubicación en los diagramas color-magnitud y período-luminosidad indican que su clasificación debe ser Cefeida Anómala.

We present spectroscopic observations of the double-lined Algol type eclipsing binary V1898 Cyg. Analyses of the BV light curves and RVs led to determination of the fundamental stellar parameters of the V1898 Cyg's components. The absolute parameters for the stars are derived as: M1 = 6.054 ± 0.037 ΜΘ, M2 = 1.162 ± 0.011 ΜΘ, R1 = 3.526 ± 0.009 RΘ, R2 = 2.640 ± 0.010 RΘ, Teff1 = 18000 ± 600 K, and Teff2 = 6200±200 K. The residuals between the observed and computed times of mid-eclipses were analysed and a rate of the period change P/P= 6.68 x 10-7 yr-1 was obtained; a mass transfer rate of 1.88 x 10-7 M0 in a year is estimated. We have calculated the distance to the system V1898Cyg as 501 ± 5 pc using the infrared JHK magnitudes and bolometric corrections for the primary star. The components of the system's proper motions present some indications about membership to the North America nebula.

Presentamos observaciones espectroscopicas de la binaria eclipsante tipo Algol, de doble linea, V1898 Cygni. El análisis de las curvas de luz en las bandas BV nos lleva a una determinación de los parámetros fundamentales de las componentes de V1898 Cygni. Los parámetros absolutos son: M1 = 6.054 ± 0.037 ΜΘ, M2 = 1.162 ± 0.011 ΜΘ, R1 = 3.526 ± 0.009 RΘ, R2 = 2.640 ± 0.010 RΘ, Teff1 = 18000 ± 600 K, y Teff2 = 6200 ± 200 K. Analizamos los residuos entre los tiempos observados y calculados para el eclipse medio y obtenemos una tasa de cambio del período de P/P= 6.68 x 10-7 yr-1. Estimamos una tasa de transferencia de masa de 1.88 x 10-7 ΜΘ por año. Utilizando las magnitudes infrarojas JHK y las correcciones bolometricas para la estrella primaria, calculamos la distancia al sistema V1898 Cyg como 501 ± 5 pc. Las componentes de los movimientos propios del sistema presentan alguna información sobre su pertenencia a la Nebulosa de Norteamerica.