activity
20232026
most citedThe Corona Australis star formation complex is accelerating away from the Galactic plane

22 citations · 51 across the 7 of their papers we have counts for

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Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2026

HURACAN: A comparison of stellar and interstellar proper motions inside L1688

M. Piecka, J. Alves, A. Rottensteiner +3

The assumption that molecular clouds are kinematically coupled to the young stellar populations forming within them is observationally still poorly constrained. With the transverse…

astro-ph.GA2026

Accelerated gas flow along Ophiuchus B44 filament: Breaking Position-Position-Velocity degeneracy

J. Alves, C. Zucker, C. Lada +15

(Abridged) Stellar feedback from massive stars in the Upper-Sco has been proposed to have reshaped the gas in the nearby Ophiuchus complex. In this framework, feedback organizes th…

astro-ph.GA20251 cited

Direct measurement of ISM proper motion with image registration

M. Piecka, L. Posch, S. Meingast +3

To date, quantification of the on-sky motion for interstellar clouds have relied on proxies such as young stellar objects (YSO) and masers. We present the first direct measurement…

astro-ph.GA20251 cited

The velocity field of the Scorpius-Centaurus OB association

S. Hutschenreuter, J. Alves, L. Posch +5

We present a non-parametric reconstruction of the three-dimensional velocity field of the Scorpius-Centaurus OB association (Sco- Cen). Using Gaia DR3 astrometry and radial velocit…

astro-ph.GA202416 cited

The physical properties of Cluster Chains

Laura Posch, João Alves, Nuria Mirét-Roig +5

We explore the kinematics and star formation history of the Scorpius Centaurus (Sco-Cen) OB association following the initial identification of sequential, linearly aligned chains…

astro-ph.GA2024

The "C": The large Chameleon-Musca-Coalsack cloud

Gordian Edenhofer, João Alves, Catherine Zucker +2

Recent advancements in 3D dust mapping have transformed our understanding of the Milky Way's local interstellar medium, enabling us to explore its structure in three spatial dimens…