2 research outputs found
Schwannoma Retroperitoneal Maligno
O schwannoma ou neurilenoma é um tumor raro que se desenvolve nas células de Schwann, na bainha dos nervos periféricos, tem crescimento lento, e pouca ou nenhuma sintomatologia, passando despercebido por um longo período. A finalidade deste trabalho é relatar dois casos de schwannoma maligno do retroperitônio, observados e tratados em nosso Serviço, bem como uma breve revisão da literatura à respeito desta patologia
CARMENES input catalog of M dwarfs: VII. New rotation periods for the survey stars and their correlations with stellar activity
Abridged: We measured photometric and spectroscopic for a large
sample of nearby bright M dwarfs with spectral types from M0 to M9, as part of
our continual effort to fully characterize the Guaranteed Time Observation
programme stars of the CARMENES survey. We determine for 129
stars. Combined with the literature, we tabulate for 261 stars,
or 75% of our sample. We evaluate the plausibility of all periods available for
this sample by comparing them with activity signatures and checking for
consistency between multiple measurements. We find that 166 of these stars have
independent evidence that confirmed their . There are
inconsistencies in 27 periods, which we classify as debated. A further 68
periods are identified as provisional detections that could benefit from
independent verification. We provide an empirical relation for the uncertainty as a function of the value, based on the
dispersion of the measurements. We show that published formal errors seem to be
often underestimated for periods d. We highlight the importance of
independent verification on measurements, especially for inactive
M dwarfs. We examine rotation-activity relations with emission in X-rays,
H, Ca II H & K, and surface magnetic field strengths. We find overall
agreement with previous works, as well as tentative differences in the
partially versus fully convective subsamples. We show as a
function of stellar mass, age, and galactic kinematics. With the notable
exception of three transiting planet systems and TZ Ari, all known planet hosts
in this sample have d. This indicates that important
limitations need to be overcome before the radial velocity technique can be
routinely used to detect and study planets around young and active stars.Comment: Accepted for publication in A&