19 research outputs found
VLBA determination of the distance to nearby star-forming regions I. The distance to T Tauri with 0.4% accuracy
In this article, we present the results of a series of twelve 3.6-cm radio
continuum observations of T Tau Sb, one of the companions of the famous young
stellar object T Tauri. The data were collected roughly every two months
between September 2003 and July 2005 with the Very Long Baseline Array (VLBA).
Thanks to the remarkably accurate astrometry delivered by the VLBA, the
absolute position of T Tau Sb could be measured with a precision typically
better than about 100 micro-arcseconds at each of the twelve observed epochs.
The trajectory of T Tau Sb on the plane of the sky could, therefore, be traced
very precisely, and modeled as the superposition of the trigonometric parallax
of the source and an accelerated proper motion. The best fit yields a distance
to T Tau Sb of 147.6 +/- 0.6 pc. The observed positions of T Tau Sb are in good
agreement with recent infrared measurements, but seem to favor a somewhat
longer orbital period than that recently reported by Duchene et al. (2006) for
the T Tau Sa/T Tau Sb system.Comment: 24 pages, 3 pages, AASTEX format, accepted for publication in Ap
HST/WFPC2 Study of the Trapezium Cluster: the Influence of Circumstellar Disks on the Initial Mass Function
We have performed the first measures of mass accretion rates in the core of
the Orion Nebula Cluster. Four adjacent fields centered on the Trapezium stars
have been imaged in the U- and B-bands using the Wide Field Planetary Camera 2
on board the Hubble Space Telescope. In this paper we focus our attention on a
group of 40 stars with known spectral types and complete UBVI WFPC2 photometry.
Approximately three quarters of the sources show excess luminosity in the
U-band, that we attribute to mass accretion. The known correlation between the
U-band excess and the total accretion luminosity allows us to estimate the
accretion rates. Overall, mass accretion rates appear lower than those measured
by other authors in the Orion flanking fields or in Taurus-Auriga. Mass
accretion rates remain low even in the vicinity of the birth line of Palla &
Stahler, suggesting that in the core of the Trapezium cluster disk accretion
has been recently depressed by an external mechanism. We suggest that the UV
radiation generated by the Trapezium OB stars, responsible for the disk
evaporation, may also cause the drop of the mass accretion rate. In this
scenario, low-mass stars may terminate their pre-main sequence evolution with
masses lower than those they would have reached if disk accretion could have
proceeded undisturbed until the final disk consumption. In OB associations the
low-mass end of the Initial Mass Function may therefore be affected by the
rapid evolution of the most massive cluster's stars, causing a surplus
"accretion aborted" very low-mass stars and brown dwarfs, and a deficit of
intermediate mass stars. This trend is in agreement with recent observations of
the IMF in the Trapezium cluster.Comment: 24 pages, 12 figures, 4 table