79 citations
- Max Planck Institute for AstronomyDE5 papers
- Ausonius Institut de Recherche sur l'Antiquité et le Moyen ageFR4 papers
- California Institute of TechnologyUS4 papers
- Max Planck Institute for Software SystemsDE4 papers
- University of CologneDE4 papers
- Center for Astrophysics Harvard & SmithsonianUS3 papers
- Commonwealth Scientific and Industrial Research OrganisationAU3 papers
- Instituto de Astrofísica de AndalucíaES3 papers
- Netherlands Institute for Radio AstronomyNL3 papers
- Tata Institute of Fundamental ResearchIN3 papers
- Aalto UniversityFI2 papers
- Chalmers University of TechnologySE2 papers
43 papers
G183: An outer galaxy filament feeding a massive protostar
Bhaswati Mookerjea, Saurav Sen, V. S. Veena +1
We present the first detailed multi-tracer observation of a 5-pc long outer Galaxy filament, G183, and the massive young stellar object (YSO) IRAS 05480+2545 associated with it. Us…
Public Opinions About Copyright for AI-Generated Art: The Role of Egocentricity, Competition, and Experience
Gabriel Lima, Nina Grgić-Hlača, Elissa Redmiles
Breakthroughs in generative AI (GenAI) have fueled debates concerning the artistic and legal status of AI-generated creations. We investigate laypeople's perceptions ()…
First detection of the [CII] 158 micron line in the intermediate-velocity cloud Draco
N. Schneider, V. Ossenkopf-Okada, E. Keilmann +7
High-latitude intermediate-velocity clouds (IVCs) are part of the Milky Way's HI halo and originate from either a galactic fountain process or extragalactic gas infall. They are pa…
Kinematics Star Formation in the Hub-Filament System G6.55-0.1
Saurav Sen, Bhaswati Mookerjea, Rolf Guesten +2
Hub-filament systems (HFSs) being the potential sites of formation of star clusters and high mass stars, provide a test bed for the current theories that attempt to explain star fo…
A Collection of German Science Interests in the Next Generation Very Large Array
M. Kadler, D. A. Riechers, J. Agarwal +88
The Next Generation Very Large Array (ngVLA) is a planned radio interferometer providing unprecedented sensitivity at wavelengths between 21 cm and 3 mm. Its 263 antenna element ar…
Constraining the geometry of the reflection nebula NGC 2023 with [O I]: Emission & Absorption
Bhaswati Mookerjea, Goeran Sandell, Rolf Guesten +3
We have mapped the NGC 2023 reflection nebula in the 63 and 145 micron transitions of [O I] and the 158 micron [C II] spectral lines using the heterodyne receiver upGREAT on SOFIA.…