2k citations
- T. Henning8 profiles80 · h 104
- E. Schinnerer2 profiles48 · h 92
- F. Walter6 profiles45 · h 100
- H. Rix2 profiles41 · h 143
- W. Brandner4 profiles41 · h 53
- N. Scoville4 profiles32 · h 93
- H. Beuther4 profiles29 · h 52
- K. Meisenheimer3 profiles28 · h 60
- C. Carilli2 profiles27 · h 92
- C. Dullemond2 profiles26 · h 82
- P. Capak2 profiles23 · h 107
- A. Pasquali3 profiles22 · h 36
- California Institute of TechnologyUS116 papers
- European Southern ObservatoryCL100 papers
- University of ArizonaUS100 papers
- Centre National de la Recherche ScientifiqueFR91 papers
- Max Planck SocietyDE82 papers
- Center for Astrophysics Harvard & SmithsonianUS76 papers
- Leiden UniversityNL71 papers
- Space Telescope Science InstituteUS71 papers
- Max Planck Institute for Extraterrestrial PhysicsDE70 papers
- National Radio Astronomy ObservatoryUS53 papers
- University of CambridgeGB47 papers
- Laboratoire d’Astrophysique de MarseilleFR43 papers
49 papers · 1 filter
GRAVITY: beam stabilization and light injection subsystems
O. Pfuhl, M. Haug, F. Eisenhauer +9
We present design results of the 2nd generation VLTI instrument GRAVITY beam stabilization and light injection subsystems. Designed to deliver micro-arcsecond astrometry, GRAVITY r…
A lower radius and mass for the transiting extrasolar planet HAT-P-8b
L. Mancini, J. Southworth, S. Ciceri +10
Context. The extrasolar planet HAT-P-8 b was thought to be one of the more inflated transiting hot Jupiters. Aims. By using new and existing photometric data, we computed precise e…
Spectral Fingerprints of Earth-like Planets Around FGK Stars
Sarah Rugheimer, Lisa Kaltenegger, Andras Zsom +2
We present model atmospheres for an Earth-like planet orbiting the entire grid of main sequence FGK stars with effective temperatures ranging from Teff = 4250K to Teff = 7000K in 2…
Tracing large-scale structures in circumstellar disks with ALMA
Jan Philipp Ruge, Sebastian Wolf, Ana L. Uribe +1
Planets are supposed to form in circumstellar disks. The gravitational potential of a planet perturbs the disk and leads to characteristic structures, i.e. spiral waves and gaps, i…
The standard model of low-mass star formation applied to massive stars: a multi-wavelength picture of AFGL 2591
K. G. Johnston, D. S. Shepherd, T. P. Robitaille +1
This paper aims to investigate the hypothesis that the embedded luminous star AFGL2591-VLA3 (2.3E5Lsun at 3.33kpc) is forming according to a scaled-up version of a low-mass star fo…
Supergiant Shells and Molecular Cloud Formation in the LMC
J. R. Dawson, N. M. McClure-Griffiths, T. Wong +4
We investigate the influence of large-scale stellar feedback on the formation of molecular clouds in the Large Magellanic Cloud (LMC). Examining the relationship between HI and 12C…