{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,11,21]],"date-time":"2025-11-21T06:09:13Z","timestamp":1763705353409,"version":"3.37.3"},"reference-count":60,"publisher":"EDP Sciences","license":[{"start":{"date-parts":[[2017,11,28]],"date-time":"2017-11-28T00:00:00Z","timestamp":1511827200000},"content-version":"vor","delay-in-days":27,"URL":"https:\/\/www.edpsciences.org\/en\/authors\/copyright-and-licensing"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["A&amp;A"],"accepted":{"date-parts":[[2017,8,29]]},"published-print":{"date-parts":[[2017,11]]},"abstract":"<jats:p><jats:italic>Context. <\/jats:italic>We map the interstellar medium (ISM) including the diffuse interstellar bands (DIBs) in absorption toward the globular cluster NGC\u20096397 using VLT\/MUSE. Assuming the absorbers are located at the rim of the Local Bubble we trace structures on the order of mpc (milliparsec, a few thousand AU). <\/jats:p>\n        <jats:p><jats:italic>Aims. <\/jats:italic>We aimed to demonstrate the feasibility to map variations of DIBs on small scales with MUSE. The sightlines defined by binned stellar spectra are separated by only a few arcseconds and we probe the absorption within a physically connected region. <\/jats:p>\n        <jats:p><jats:italic>Methods. <\/jats:italic>This analysis utilized the fitting residuals of individual stellar spectra of NGC\u20096397 member stars and analyzed lines from neutral species and several DIBs in Voronoi-binned composite spectra with high signal-to-noise ratio (S\/N). <\/jats:p>\n        <jats:p><jats:italic>Results. <\/jats:italic>This pilot study demonstrates the power of MUSE for mapping the local ISM on very small scales which provides a new window for ISM observations. We detect small scale variations in Na I\u2009and K I\u2009as well as in several DIBs within few arcseconds, or mpc with regard to the Local Bubble. 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