Fabian Walter

TL;DR: In this paper, the authors investigated the origins of [C II] emission by examining high spatial resolution observations of star-forming galaxies with the Survey of Lines in M31 and found that a significant amount (~20%-90%) of the emission comes from outside star forming regions and the total IR emission (TIR) has the highest diffuse fraction of all SFR tracers.

TL;DR: In this article, the authors analyzed line-of-sight atomic hydrogen (HI) line profiles of 31 nearby, low-mass galaxies selected from the VLA-ANGST and The HI Nearby Galaxy Survey (THINGS) to trace regions containing cold (T$ 1400 K) HI from observations with a uniform linear scale of 200 pc/beam.

TL;DR: In this article, a comprehensive study of the star cluster population and the hierarchical structure in the clustering of blue stars with ages <500 Myr in the Local Group dwarf irregular galaxy NGC 6822 is presented.

TL;DR: In this paper, high-resolution H I observations obtained with the Very Large Array, as well as optical broadband imaging, of the dwarf irregular galaxy DDO 47 (UGC 3974, CGCG 087-030) were presented.

TL;DR: In this paper, the authors proposed a method to improve the performance of the National Aeronautics and Space Administration (NNX08AR22G), National Science Foundation (NSF), and the Ministry of Science and Technology (MoST) of Taiwan through grant National Science Council (NSC) and MoST of Taiwan.