Dopamine signaling is essential in cognitive process and motor performance

La dopamina es uno de los principales neurotransmisores del sistema nervioso central y desempeña un papel esencial en diferentes funciones: neuroendocrinas, motivacionales/emocionales y, especialmente, motoras y cognitivas. Las funciones de la dopamina están media-das en gran medida por la estimulación de sus principales receptores D1 (D1R) y D2 (D2R). En esta tesis hemos estudiado el papel que ambos receptores desempeñan en los procesos de apren-dizaje y memoria, así como la regulación que ejercen sobre las neuronas estriatales TH-immunoreactivas (TH-ir) y su posible implicación en la respuesta motora. Para abordar este proyecto hemos utilizado ratones knock-out para el receptor D1 (Drd1a-/-) y D2 (Drd2-/-) ya que no existen compuestos farmacológicos capaces de diferenciar eficazmente entre receptores dopaminérgicos de la misma familia. Además, para el estudio de las neuronas TH-ir realizamos lesiones con 6-OHDA a ratones que posteriormente recibieron un tratamiento crónico con L-DOPA, siendo este el mecanismo más eficaz para inducir la expresión de las neuronas TH-ir objeto de nuestro estudio. Para completar todo ello realizamos test conductuales que evalúan respuesta motora, como el test del cilindro, y diferentes tipos de aprendizaje y me-moria para los cuales utilizamos test específicos. Entre estos test se encuentran: los laberintos de Barnes y Morris para memoria espacial, evitación activa/pasiva y condicionamiento del mie-do para el aprendizaje asociativo, y el reconocimiento de objetos para la memoria de reconoci-miento...

FR Cnc revisited: photometry, polarimetry and spectroscopy

This paper is part of a multiwavelength study aimed at using complementary photometric, polarimetric and spectroscopic data to achieve an understanding of the activity process in late-type stars. Here, we present the study of FR Cnc, a young, active and spotted star. We performed analysis of All Sky Automated Survey 3 (ASAS-3) data for the years 2002–08 and amended the value of the rotational period to be 0.826518 d. The amplitude of photometric variations decreased abruptly in the year 2005, while the mean brightness remained the same, which was interpreted as a quick redistribution of spots. BVR_C and I_C broad-band photometric calibration was performed for 166 stars in FR Cnc vicinity. The photometry at Terskol Observatory shows two brightening episodes, one of which occurred at the same phase as the flare of 2006 November 23. Polarimetric BVR observations indicate the probable presence of a supplementary source of polarization. We monitored FR Cnc spectroscopically during the years 2004–08. We concluded that the radial velocity changes cannot be explained by the binary nature of FR Cnc. We determined the spectral type of FR Cnc as K7V. Calculated galactic space-velocity components (U, V, W) indicate that FR Cnc belongs to the young disc population and might also belong to the IC 2391 moving group. Based on Li Iλ6707.8 measurement, we estimated the age of FR Cnc to be between 10 and 120 Myr. Doppler tomography was applied to create a starspot image of FR Cnc. We optimized the goodness of fit to the deconvolved profiles for axial inclination, equivalent width and v sin i, finding v sin  i=46.2 km s^−1 and i= 55°. We also generated a syntheticV-band light curve based on Doppler imaging that makes simultaneous use of spectroscopic and photometric data. This synthetic light curve displays the same morphology and amplitude as the observed one. The starspot distribution of FR Cnc is also of interest since it is one of the latest spectral types to have been imaged. No polar spot was detected on FR Cnc.