activity
20172021
most citedThe asymmetric inner disk of the Herbig Ae star HD 163296 in the eyes of VLTI/MATISSE: evidence for a vortex?

43 citations · 73 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.EP202112 cited

First MATISSE L-band observations of HD 179218. Is the inner 10 au region rich in carbon dust particles?

E. Kokoulina, A. Matter, B. Lopez +58

Carbon is one of the most abundant components in the Universe. While silicates have been the main focus of solid phase studies in protoplanetary discs (PPDs), little is known about…

astro-ph.SR2021

Mid-infrared circumstellar emission of the long-period Cepheid l Carinae resolved with VLTI/MATISSE

V. Hocdé, N. Nardetto, A. Matter +149

The nature of circumstellar envelopes (CSE) around Cepheids is still a matter of debate. The physical origin of their infrared (IR) excess could be either a shell of ionized gas, o…

astro-ph.SR202043 cited

The asymmetric inner disk of the Herbig Ae star HD 163296 in the eyes of VLTI/MATISSE: evidence for a vortex?

J. Varga, M. Hogerheijde, R. van Boekel +133

Context. The inner few au region of planet-forming disks is a complex environment. High angular resolution observations have a key role in understanding the disk structure and the…

astro-ph.IM20189 cited

Why Chromatic Imaging Matters

Joel Sanchez-Bermudez, Florentin Millour, Fabien Baron +15

During the last two decades, the first generation of beam combiners at the Very Large Telescope Interferometer has proved the importance of optical interferometry for high-angular…

astro-ph.GA2018

Flat Rotation Curves found in Merging Dusty Starbursts at through Tilted-Ring Modeling

Rui Xue, Hai Fu, Jacob Isbell +3

The brightest 500m source in the XMM field, HXMM01, is a rare merger of luminous starburst galaxies at with a dust-obscured star-formation rate of 2,000$\,M_{\odot}\,{…

astro-ph.GA2018

SDSS-IV MaNGA: Galaxy Pair Fraction and Correlated Active Galactic Nuclei

Hai Fu, Joshua L. Steffen, Arran C. Gross +7

We have identified 105 galaxy pairs at z ~ 0.04 with the MaNGA integral-field spectroscopic data. The pairs have projected separations between 1 kpc and 30 kpc, and are selected to…