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M. Habibi

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • last author2

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
ORCID 0000-0003-1366-1695
same name
  • M. Habibi — 29 papers, h 28
  • M. Habibi — 6 papers, h 11
  • M. Habibi — 5 papers, h 24
  • M. Habibi — 2 papers, h 11
  • M. Habibi — 1 paper
  • M. Habibi — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedThe mass distribution in the Galactic Centre from interferometric astrometry of multiple stellar orbits

287 citations · 322 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2021★ 287 cited

The mass distribution in the Galactic Centre from interferometric astrometry of multiple stellar orbits

GRAVITY Collaboration, R. Abuter, N. Aimar +62

The stars orbiting the compact radio source Sgr A* in the Galactic Centre are precision probes of the gravitational field around the closest massive black hole. In addition to adap…

astro-ph.GA2021★ 35 cited

Deep Images of the Galactic Center with GRAVITY

GRAVITY Collaboration, R. Abuter, N. Aimar +65

Stellar orbits at the Galactic Center provide a very clean probe of the gravitational potential of the supermassive black hole. They can be studied with unique precision, beyond th…

astro-ph.GA2016

3D AMR simulations of G2 as an outflow

A. Ballone, M. Schartmann, A. Burkert +8

We study the evolution of G2 in a \textit{Compact Source Scenario}, where G2 is the outflow from a low-mass central star moving on the observed orbit. This is done through 3D AMR s…

astro-ph.GA2016

3D AMR simulations of the evolution of the diffuse gas cloud G2 in the Galactic Centre

M. Schartmann, A. Ballone, A. Burkert +8

With the help of 3D AMR hydrodynamical simulations we aim at understanding G2's nature, recent evolution and fate in the coming years. By exploring the possible parameter space of…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.