Maryam Habibi
Max Planck Society
76 Papers
936 Citations
Maryam Habibi is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galactic Center & Stars. The author has an hindex of 27, co-authored 73 publications. Previous affiliations of Maryam Habibi include University of Bonn.
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Papers
A parameter survey of Sgr A∗ radiative models from GRMHD simulations with self-consistent electron heating
Jason Dexter,Jason Dexter,A. Jiménez-Rosales,S M Ressler,Alexander Tchekhovskoy,M. Bauböck,P. T. de Zeeuw,Frank Eisenhauer,S. von Fellenberg,Feng Gao,Reinhard Genzel,Reinhard Genzel,Stefan Gillessen,Maryam Habibi,T. Ott,Julia Stadler,Odele Straub,Felix Widmann +17 more
TL;DR: In this paper, the authors compare images and spectra generated from a parameter survey of general relativistic MHD simulations to a set of radio to NIR observations of Sgr A*, and find two classes of scenarios can explain the broad shape of the submillimetre spectral peak and the highly variable NIR flaring emission.
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Detection of a drag force in G2's orbit: Measuring the density of the accretion flow onto Sgr A* at 1000 Schwarzschild radii
Stefan Gillessen,P. M. Plewa,Felix Widmann,S. von Fellenberg,Marc Schartmann,Maryam Habibi,A. Jimenez Rosales,M. Bauböck,Jason Dexter,Feng Gao,I. Waisberg,Frank Eisenhauer,Oliver Pfuhl,Thomas Ott,Andreas Burkert,P. T. de Zeeuw,P. T. de Zeeuw,Reinhard Genzel,Reinhard Genzel +18 more
TL;DR: In this paper, the authors used the dynamics of the gas cloud G2 to probe the ambient density at around 1000 Schwarzschild radii and yields a number density of approx. 4 x 10^3 cm^-3.
The Flux Distribution of Sgr A
Roberto Abuter,António Amorim,M. Bauböck,J. B. Berger,J. B. Berger,H. Bonnet,Wolfgang Brandner,Vitor Cardoso,Yann Clénet,P. T. de Zeeuw,Y. Dallilar,Jason Dexter,Andreas Eckart,Andreas Eckart,Frank Eisenhauer,N. M. Förster Schreiber,Paulo J. V. Garcia,Paulo J. V. Garcia,Feng Gao,Eric Gendron,Reinhard Genzel,Stefan Gillessen,Maryam Habibi,Xavier Haubois,Th. Henning,Stefan Hippler,Matthew Horrobin,A. Jiménez-Rosales,Lieselotte Jochum,Laurent Jocou,Andreas Kaufer,Pierre Kervella,Sylvestre Lacour,Sylvestre Lacour,V. Lapeyrère,J.-B. Le Bouquin,Pierre Léna,M. Nowak,Thomas Ott,Thibaut Paumard,Karine Perraut,Guy Perrin,Oliver Pfuhl,Gabriele Ponti,G. Rodriguez Coira,Jinyi Shangguan,Silvia Scheithauer,Julia Stadler,Odele Straub,Christian Straubmeier,Eckhard Sturm,Linda J. Tacconi,F. Vincent,S. D. von Fellenberg,I. Waisberg,Felix Widmann,Ekkehard Wieprecht,Erich Wiezorrek,Julien Woillez,Senol Yazici,Gérard Zins +60 more
TL;DR: In this paper, the authors used the GRAVITY instrument at the VLTI to measure the median flux density, and to test if the previously proposed flux distributions fit the data, and obtained light curves using interferometric model fitting and coherent flux measurements.
The orbital motion of the quintuplet cluster—a common origin for the arches and quintuplet clusters?*
A. Stolte,B. Hußmann,Mark Morris,Andrea M. Ghez,Wolfgang Brandner,Jessica R. Lu,Will Clarkson,Maryam Habibi,Keith Matthews +8 more
TL;DR: In this paper, the authors investigated the orbital motion of the Quintuplet cluster near the Galactic center with the aim of constraining formation scenarios of young, massive star clusters in nuclear environments.
Isolated massive stars in the Galactic center: The dynamic contribution from the Arches and Quintuplet star clusters
TL;DR: In this paper, the distribution of drifted sources in numerical models of the massive clusters in the Galactic center and compare it to the observed distribution of isolated massive sources in this region was investigated.