Hans-Walter Rix How Can a 3D-Map of Dust Help Measure Distances in our Milky Way?

Hans-Walter Rix is Director at the Max Planck Institute for Astronomy in Heidelberg; he is also an Honorary Professor at the University of Heidelberg in Germany. Upon completion of his PhD at the University of Arizona (Tucsan) he was awarded a Hubble Fellowship, which he took to the Institute for Advanced Studies in Princeton. There, he worked on some of the first Hubble Space Telescope data on gravitational lensing. His fields of research are galaxy evolution and galaxy structure, which he investigates by means of spectroscopic and imaging surveys, currently focusing on the Milky Way as a "galaxy model organism". Rix is a member of the German National Academy of Sciences, the Leopoldina.

Area of Research

Astronomy

Henrik Beuther, Ralf S. Klessen, Cornelis P. Dullemond and Thomas Henning (Eds.). Protostars and Planets VI. 2014.  
Jo Bovy, Hans-Walter Rix and David W. Hogg. "The Milky Way Has No Distinct Thick Disk." The Astrophysical Journal 751 (2012): No. 131.  
Hans-Walter Rix and Jo Bovy. "The Milky Way's Stellar Disk. Mapping and Modeling the Galactic Disk." Astronomy and Astrophysics Review 21, 1 (2013): No. 61.  
Jo Bovy and Hans-Walter Rix. "A Direct Dynamical Measurement of the Milky Way's Disk Surface Density Profile, Disk Scale Length, and Dark Matter Profile at 4 kpc≲ R≲ 9 kpc." The Astrophysical Journal 779, 2 (2013).  
Edward Churchwell, Brian L. Babler, Marilyn R. Meade, Barbara A. Whitney, Robert Benjamin, Remy Indebetouw, Claudia Cyganowski, Thomas P. Robitaille, Matthew Povich and Christer Watson. "The Spitzer/GLIMPSE Surveys: A New View of the Milky Way." Publications of the Astronomical Society of the Pacific 121 (2009): No. 213.  
Edward Schlafly, Gregory Green, Douglas Finkbeiner, Hans-Walter Rix, Eric Bell, William Burgett, Ken Chambers, Peter Draper, Klaus Werner Hodapp and Nick Kaiser. "A Large Catalog of Accurate Distances to Molecular Clouds from PS1 Photometry." The Astrophysical Journal 786 (2014): No. 29.  
Edward Schlafly, Gregory Green, Douglas Finkbeiner, Mario Jurić, Hans-Walter Rix, Nicholas Martin, William Burgett, Ken Chambers, Peter Draper and Klaus Werner Hodapp. "A Map of Dust Reddening to 4.5 kpc from Pan-STARRS1." The Astrophysical Journal 789 (2014): No. 15.  
Edward Schlafly, Aaron Meisner, Amelia Stutz, Jouni Kainulainen, Joshua Peek, Oleg Tchernyshyov, Hans-Walter Rix, Douglas Finkbeiner, Kevin Covey and Gregory Green. "The Optical–Infrared Extinction Curve and its Variation in the Milky Way." The Astrophysical Journal 821 (2016): No. 78.  
Hans-Walter Rix, P. Tim De Zeeuw, Nicolas Cretton, Roeland P. van der Marel and C. Marcella Carollo. "Dynamical Modeling of Velocity Profiles: The Dark Halo Around the Elliptical Galaxy ngc 2434." The Astrophysical Journal 488 (1997): No. 702.  
Hans-Walter Rix, Marco Barden, Steven V. W. Beckwith, Eric F. Bell, Andrea Borch, John A. R. Caldwell, Boris Häussler, Knud Jahnke, Shardha Jogee and Daniel H. McIntosh. "GEMS: Galaxy Evolution from Morphologies and SEDs." The Astrophysical Journal Supplement Series 152 (2004): No. 163.  
Hans-Walter Rix and Jo Bovy. "The Milky Way’s Stellar Disk." The Astronomy and Astrophysics Review 21 (2013): No. 61.  

since 1999

Director

Max Planck Society (more details)

Max Planck Institute for Astronomy

since 2000

Honorary Professor

Heidelberg University (Ruprecht-Karls-Universität Heidelberg)

1998-1999

Associate Professor

University of Arizona

1995-1998

Assistant Professor/Astronome

University of Arizona

1994-1995

Research Scientist

Max Planck Society (more details)

Max Planck Institute for Astrophysics

1991-1994

Member

Institute for Advanced Study

1986-1991

PhD

University of Arizona

Member of the German National Academy of Sciences Leopoldina

Member of the European Academy of Sciences and Arts

Prizes

ERC Advanced Grant Award (2013-2018)

Fellowships

Alfred P. Sloan Fellowship (1996-1998)

Hubble Fellowship at the Institute for Advanced Study, Princeton (1991-1994)

© Maximilian Dörrbecker

Max Planck Society


"The Max Planck Society is Germany's most successful research organization. Since its establishment in 1948, no fewer than 18 Nobel laureates have emerged from the ranks of its scientists, putting it on a par with the best and most prestigious research institutions worldwide. The more than 15,000 publications each year in internationally renowned scientific journals are proof of the outstanding research work conducted at Max Planck Institutes – and many of those articles are among the most-cited publications in the relevant field." (Source)

Institute

Max Planck Institute for Astronomy

How do stars and planets form? What can we learn about planets orbiting stars other than the Sun? How do galaxies form, and how have they changed in the course of cosmic history?

Those are the central questions guiding the work of the scientists and engineers at the Max Planck Institute for Astronomy (MPIA) in Heidelberg. The institute was founded in 1967, and it is one of roughly 80 institutes of the Max Planck Society, Germany's largest organizations for basic research.

MPIA has a staff of around 290, three quarters of which are working in sci-tech. At any given time, the institute features numerous junior scientists and guest scientists both from Germany and abroad. (Source)

Map

The dust in our Milky Way is the constituent of the cosmic life cycle. It is the substance from which new stars are generated and it is what stars become once they die. Unfortunately, as HANS-WALTER RIX explains in this video, the dust turns distance measurements of stars in the Milky Way into a difficult endeavor, because it dims objects and blocks light from the material behind it. In his project two common methods of distance measurement are therefore used in combination to sketch a 3D map of Milky Way dust: first the parallax, which uses the orbit character of the earth in order to check on the stars’ respective positions, and second, the calculated brightness of stars which allows for an estimate concerning the amount of dust in front of each star. The so created 3D map helps to limit errors in distance calculations due to a feasible dust exclusion, made possible by the localization of dust. The conversion of observed quantities into physical quantities thus becomes possible.

LT Video Publication DOI: http://dx.doi.org/10.21036/LTPUB10369

A Three-dimensional Map of Milky Way Dust

  • Gregory M. Green, Edward F. Schlafly, Douglas P. Finkbeiner, Hans-Walter Rix, Nicolas Martin, William Burgett, Peter W. Draper, Heather Flewelling, Klaus Hodapp and Nicholas Kaiser
  • The Astrophysical Journal
  • Published in 2015

Chicago

Gregory M. Green, Edward F. Schlafly, Douglas P. Finkbeiner, Hans-Walter Rix, Nicolas Martin, William Burgett, Peter W. Draper, Heather Flewelling, Klaus Hodapp and Nicholas Kaiser. "A Three-dimensional Map of Milky Way Dust." The Astrophysical Journal 810 (2015): 25.