| The process of star formation involves several simultaneous physical processes such as accretion, ejection and outbursts affecting the disk and the subsequent outflows emerging from the host star. Recent studies have concluded that star-forming regions are composed of a population of stars as well as sub-stellar regime objects as a function of its environment. Observations of YSOs enshrouded by dust and gas in stellar nurseries provide opportunities to study the intricate details of such environments where several dynamical processes simultaneously affect the physical and chemical structure of the stellar nursery. One such process being outflows from early-stage protostars as they launch powerful jets and outflows that are capable of regulating the angular momentum of the star as it accretes matter but also altering the physical and chemical structure of its immediate environment. Outflows are thus key parameters in several unanswered questions of star formation. Previous studies have modeled bipolar outflows as conical structures, aiming to measure their opening angles to better understand the physical mechanisms driving their evolution in star-forming regions like Perseus. In this talk, I present preliminary findings from the CAMPOS ALMA Band 6 survey of Class 0/I low-mass protostars in several nearby star-forming regions. Our analysis focuses on the evolution of bipolar outflows and their morphological transformation as a function of the protostellar age, with bolometric temperature serving as a key evolutionary proxy, for selected protostars in the Aquila and Serpens star-forming regions located at 436 pc. We examine the changing opening angles of the outflows, comparing the red- and blue-shifted velocity lobes, from their launch regions to the outermost extents to understand how the outflows vary radially as well as the asymmetries present within the blue and red shifted lobes themselves. |
