Closer galaxies like the Magellanic Clouds, M31, or M33 do not allow similar large-scale multiwavelength mapping due to their large angular sizes, while more distant galaxies (beyond a few Mpc) do not allow multiwavelength studies with similar spatial resolution across the optical, infrared, mm/sub-mm, and radio. 2019 Schruba, Kruijssen & Leroy 2019) makes NGC 300 the ideal target for simultaneous resolved feedback, stellar population, and ISM studies. 2004 Westmeier, Braun & Koribalski 2011 Riener et al. The large spatial coverage (to cover most of the star-forming disc) available not only in the optical with MUSE but throughout the electromagnetic spectrum (e.g. 2009), non-interacting, star-forming disc galaxy that can be mapped at the necessary spatial resolution. NGC 300 is an ideal target to study stellar feedback: it is the closest ( D ∼ 2 Mpc Dalcanton et al.

So saying its an old game only makes it worse, because how longer it takes to fix things the worse it is. Uhm 2560x1080 IS in the game, it just does not work. 2010), consisting of a contiguous 7 arcmin × 5 arcmin mosaic (∼4 kpc × 3 kpc) and covering the galaxy out to galactocentric radii of about 0.45 R 25 (with R 25 ∼ 5.33 kpc being the optical radius Paturel et al. You can't expect them to patch in every new aspect ratio or resolution in old games. In this paper, we use a legacy value data set covering the inner star-forming disc of NGC 300 taken with the VLT/MUSE instrument (Bacon et al. We extract spectra from emission line regions identified within dendrograms, combine emission line ratios and line widths to distinguish between |$$| regions in NGC 300 in a spatially resolved manner and find that their expansion is governed by the pressure of the ionized gas and by the winds from the massive stars within them. We use the Very Large Telescope (VLT) MUSE (Multi Unit Spectroscopic Explorer) legacy data set covering the central 35 arcmin 2 (∼12 kpc 2) of the nearby galaxy NGC 300 to quantify the effect of stellar feedback as a function of the local galactic environment.

Integral field units enable resolved studies of a large number of star-forming regions across entire nearby galaxies, providing insight on the conversion of gas into stars and the feedback from the emerging stellar populations over unprecedented dynamic ranges in terms of spatial scale, star-forming region properties, and environments.

Mass effect 1 pc resolution