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21 papers
Aspect ratios of far-infrared and H i filaments in the diffuse interstellar medium at high Galactic latitudes
P. M. W. Kalberla, U. Haud
Dusty magnetized structures observable in the far-infrared (FIR) at high Galactic latitudes are ubiquitous and found to be closely related to HI filaments with coherent velocity st…
Correlations between turbulent velocity and density fields in the local interstellar medium
P. M. W. Kalberla, J. Kerp, U. Haud
Kalberla et al. used HI4PI data to analyze velocity and density fluctuations in the interstellar medium (ISM). They applied the Yuen et al. (2021) velocity decomposition algorithm…
Local HI filaments driven by a small-scale dynamo. Update on the velocity decomposition algorithm
P. M. W. Kalberla, J. Kerp, U. Haud
Context. HI filaments are closely related to dusty magnetized structures that are observable in the far infrared (FIR). Recently it was proposed that the coherence of oriented HI s…
HI filaments are cold and associated with dark molecular gas. HI4PI based estimates of the local diffuse CO-dark H2 distribution
P. M. W. Kalberla, J. Kerp, U. Haud
Context. There are significant amounts of H2 in the Milky Way. Due to its symmetry H2 does not radiate at radio frequencies. CO is thought to be a tracer for H2, however CO is form…
Are observed H i filaments turbulent illusions or density structures? Velocity caustics, facts and fakes
P. M. W. Kalberla, U. Haud
Context. The interstellar medium is affected by turbulence and observed H i structures in channel maps are shaped by turbulent motions. It is taken for granted by a few theoreticia…
Turbulent power distribution in the local interstellar medium
P. M. W. Kalberla, U. Haud
Context: The interstellar medium (ISM) on all scales is full of structures that can be used as tracers of processes that feed turbulence. Aims: We used HI survey data to derive glo…