Eli Bressert

TL;DR: In this paper, the authors presented a detailed study of a peculiar source in the COSMOS survey at z=0.359, where the distance between the 2, measured in the HST/ACS image, is 0.495" that corresponds to a projected separation of 2.46 kpc.

TL;DR: In this article, the authors make use of existing multi-wavelength data including recently available far-IR continuum (Herschel/Hi-GAL) and mm spectral line (HOPS and MALT90) data and present new, deep, multiple-filter, near-IR (VLT/NACO) observations to study G0.253+0.016.

TL;DR: In this paper, the authors examined the evidence offered for triggered star formation against the backdrop provided by recent numerical simulations of feedback from massive stars at or below giant molecular cloud sizescales, and found that none of the observational markers improved the chances of correctly identifying a given star as triggered by more than factors of two at most.

TL;DR: In this article, the authors search the 1.1 mm Bolocam Galactic Plane Survey for clumps containing sufficient mass to form approximately 10{sup 4} M{sub Sun} star clusters and find that all massive proto-clusters in the first quadrant are actively forming massive stars.

TL;DR: In this paper, the authors estimate the observable properties of the massive proto-clusters (MPCs) for existing Galactic plane surveys and suggest how they may be sought in recent and upcoming extragalactic observations.