3D shape of Orion A with Gaia DR2. An informed view on Star Formation Rates and Efficiencies. (arXiv:1812.08024v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Grossschedl_J/0/1/0/all/0/1">Josefa E. Großschedl</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Alves_J/0/1/0/all/0/1">João Alves</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Meingast_S/0/1/0/all/0/1">Stefan Meingast</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hasenberger_B/0/1/0/all/0/1">Birgit Hasenberger</a>
The giant molecular cloud Orion A is the closest massive star-forming region
to earth ($dsim400$ pc). It contains the rich Orion Nebula Cluster (ONC) in
the North, and low-mass star-forming regions (L1641, L1647) to the South. To
get a better understanding of the differences in star formation activity, we
perform an analysis of the gas mass distribution and star formation rate across
the cloud. We find that the gas is roughly uniformly distributed, while, oddly,
the ONC region produced about a factor of ten more stars compared to the rest
of the cloud. For a better interpretation of this phenomenon, we use Gaia DR2
parallaxes, to analyse distances of young stellar objects, using them as proxy
for cloud distances. We find that the ONC region indeed lies at about 400 pc
while the low-mass star-forming parts are inclined about 70$^circ$ from the
plane of the sky reaching until $sim$470 pc. With this we estimate that Orion
A is an about 90 pc long filamentary cloud (about twice as long as previously
assumed), with its “Head” (the ONC region) being “bent” and oriented toward the
galactic mid-plane. This striking new view allows us to perform a more robust
analysis of this important star-forming region in the future.
The giant molecular cloud Orion A is the closest massive star-forming region
to earth ($dsim400$ pc). It contains the rich Orion Nebula Cluster (ONC) in
the North, and low-mass star-forming regions (L1641, L1647) to the South. To
get a better understanding of the differences in star formation activity, we
perform an analysis of the gas mass distribution and star formation rate across
the cloud. We find that the gas is roughly uniformly distributed, while, oddly,
the ONC region produced about a factor of ten more stars compared to the rest
of the cloud. For a better interpretation of this phenomenon, we use Gaia DR2
parallaxes, to analyse distances of young stellar objects, using them as proxy
for cloud distances. We find that the ONC region indeed lies at about 400 pc
while the low-mass star-forming parts are inclined about 70$^circ$ from the
plane of the sky reaching until $sim$470 pc. With this we estimate that Orion
A is an about 90 pc long filamentary cloud (about twice as long as previously
assumed), with its “Head” (the ONC region) being “bent” and oriented toward the
galactic mid-plane. This striking new view allows us to perform a more robust
analysis of this important star-forming region in the future.
http://arxiv.org/icons/sfx.gif
