High Galactic latitude runaway stars as tracers of the spiral arms
@article{Silva2013HighGL, title={High Galactic latitude runaway stars as tracers of the spiral arms}, author={M Silva and Ralf Napiwotzki}, journal={Monthly Notices of the Royal Astronomical Society}, year={2013}, volume={431}, pages={502-510} }
A direct observation of the spiral structure of the Galaxy is hindered by our position in the middle of the Galactic plane. We propose a method based on the analysis of the birthplaces of high Galactic latitude runaway stars to map the spiral arms and determine their dynamics. As a proof of concept, the method is applied to a local sample of early-type stars and a sample of runaways stars to obtain estimates of the pattern speed (p,local = 20.3 ± 0.5 kms −1 kpc −1 and p,runaway = 21.9 ± 8.6 kms…
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References
SHOWING 1-10 OF 36 REFERENCES
Kinematics of young stars. II. Galactic spiral structure
- Physics
- 2001
The young star velocity eld is analysed by means of a galactic model which takes into account solar motion, dierential galactic rotation and spiral arm kinematics. We use two samples of Hipparcos…
Ejection velocities of high Galactic latitude runaway stars
- Physics, Geology
- 2010
We estimate the distribution of ejection velocities for the known population of high Galactic latitude runaway stars. The initial sample is a collection of 174 early-type stars selected from the…
A plausible Galactic spiral pattern and its rotation speed
- Physics
- 2004
We report calculations of the stellar and gaseous response to a Milky Way mass distribution model including a spiral pattern with a locus as traced by K-band observations, superimposed on the…
DIRECT DETERMINATION OF THE SPIRAL PATTERN ROTATION SPEED OF THE GALAXY
- Physics
- 2005
The rotation velocity of the spiral pattern of the Galaxy is determined by direct observation of the birthplaces of open clusters of stars in the Galactic disk as a function of their age. Our…
The Origins and Evolutionary Status of B Stars Found Far from the Galactic Plane. II. Kinematics and Full Sample Analysis
- Physics
- 2002
This paper continues the analysis of faint high-latitude B stars from Martin. Here we analyze the kinematics of the stars and combine them with the abundance information from the first paper to…
The Nature of the Hyper-Runaway Candidate Hip 60350
- Physics
- 2010
Young, massive stars in the Galactic halo are widely supposed to be the result of an ejection event from the Galactic disk forcing some stars to leave their place of birth as so-called runaway stars.…
Early type stars at high galactic latitudes I. Ten young massive B-type stars
- Physics, Geology
- 2001
We present the results of quantitative spectral analyses of ten apparently normal B-type stars. These stars were found to be young massive B-type stars at distances of z=2.6 to 7.6 kpc from the…
The spiral structure of the Galaxy revealed by CS sources and evidence for the 4:1 resonance
- Physics
- 2010
We present a map of the spiral structure of the Galaxy, as traced by molecular carbon monosulphide (CS) emission associated with IRAS sources which are believed to be compact H ii regions. The CS…
Star-forming complexes and the spiral structure of our Galaxy
- Physics
- 2003
We have carried out a multiwavelength study of the plane of our Galaxy in order to establish a star-forming-complex catalogue which is as complete as possible. Features observed include H, H109, CO,…
On the origin of the o and b-type stars with high velocities II runaway stars and pulsars ejected from the nearby young stellar groups
- Physics
- 2001
We use milli-arcsecond accuracy astrometry (proper motions and parallaxes) from Hipparcos and from radio observations to retrace the orbits of 56 runaway stars and nine compact objects with distances…