activity
20172020
most citedThe formation of direct collapse black holes under the influence of streaming velocities

99 citations · 211 across the 6 of their papers we have counts for

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Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2020

The Ultimately Large Telescope -- what kind of facility do we need to detect Population III stars?

Anna T. P. Schauer, Niv Drory, Volker Bromm

The launch of the James Webb Space Telescope will open up a new window for observations at the highest redshifts, reaching out to z~15. However, even with this new facility, the fi…

astro-ph.GA2019

Shape and Spin of Minihaloes. II: The Effect of Streaming Velocities

Maik Druschke, Anna T. P. Schauer, Simon C. O. Glover +1

Models of the decoupling of baryons and photons during the recombination epoch predict the existence of a large-scale velocity offset between baryons and dark matter at later times…

astro-ph.GA20198 cited

Constraining the non-gravitational scattering of baryons and dark matter with early cosmic structure formation

Boyuan Liu, Anna T. P. Schauer, Volker Bromm

We derive new constraints on the non-gravitational baryon-dark-matter scattering (BDMS) by evaluating the mass thresholds of dark matter (DM) haloes in which primordial gas can coo…

astro-ph.GA201959 cited

Constraining First Star Formation with 21cm-Cosmology

Anna T. P. Schauer, Boyuan Liu, Volker Bromm

Within standard CDM cosmology, Population III (Pop III) star formation in minihalos of mass M provides the first stellar sources of…

astro-ph.GA2018

The Influence of Streaming Velocities on the Formation of the First Stars

Anna T. P. Schauer, Simon C. O. Glover, Ralf S. Klessen +1

How, when and where the first stars formed are fundamental questions regarding the epoch of Cosmic Dawn. A second order effect in the fluid equations was recently found to make a s…

astro-ph.GA2018

Shape and Spin of Minihaloes: From Large Scales to the Centres

Maik Druschke, Anna T. P. Schauer, Simon C. O. Glover +1

The spin and shape of galaxies at the present day have been well-studied both observationally and theoretically. At high redshifts, however, we have to rely on numerical simulation…