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Space Telescope and Optical Reverberation Mapping Project. XII. Broad-Line Region Modeling of NGC 5548
P. R. Williams, A. Pancoast, T. Treu +155
We present geometric and dynamical modeling of the broad line region for the multi-wavelength reverberation mapping campaign focused on NGC 5548 in 2014. The dataset includes photo…
Infrared Telescope Facility (IRTF) spectral library II: New indices in Y, J, H, and L atmospheric windows
L. Morelli, V. D. Ivanov, A. Pizzella +6
Stellar population studies in the infrared (IR) wavelength range have two main advantages with respect to the optical regime: they probe different populations, because most of the…
AlFoCS + Fornax3D: resolved star formation in the Fornax cluster with ALMA and MUSE
Nikki Zabel, Timothy A. Davis, Marc Sarzi +18
We combine data from ALMA and MUSE to study the resolved (~300 pc scale) star formation relation (star formation rate vs. molecular gas surface density) in cluster galaxies. Our sa…
The Fornax 3D project: Non-linear colour-metallicity relation of globular clusters
K. Fahrion, M. Lyubenova, M. Hilker +15
Globular cluster (GC) systems of massive galaxies often show a bimodal colour distribution. This has been interpreted as a metallicity bimodality, created by a two-stage galaxy for…
The Fornax 3D project: Globular clusters tracing kinematics and metallicities
K. Fahrion, M. Lyubenova, M. Hilker +15
Globular clusters (GCs) are found ubiquitously in massive galaxies and due to their old ages, they are regarded as fossil records of galaxy evolution. Spectroscopic studies of GC s…
Fornax 3D project: automated detection of planetary nebulae in the centres of early-type galaxies and first results
T. W. Spriggs, M. Sarzi, R. Napiwotzki +15
Extragalactic planetary nebulae (PNe) are detectable through relatively strong nebulous [OIII] emission and act as direct probes into the local stellar population. Because they hav…