From interstellar abundances to grain composition: the major dust constituents Mg, Si, and FeVOSHCHINNIKOV, N. V; HENNING, Th.Astronomy and astrophysics (Berlin. Print). 2010, Vol 517, issn 0004-6361, A45.1-A45.15Article

Multiple low-turbulence starless cores associated with intermediate- to high-mass star formationBEUTHER, H; HENNING, Th.Astronomy and astrophysics (Berlin. Print). 2009, Vol 503, Num 3, pp 859-867, issn 0004-6361, 9 p.Article

Accelerated self-consistent radiative transfer based on the Monte Carlo methodWOLF, S; HENNING, Th.Computer physics communications. 2000, Vol 132, Num 1-2, pp 166-188, issn 0010-4655Article

Massive binaries in the Cepheus OB2/3 region*: Constraining the formation mechanism of massive starsPETER, D; FELDT, M; HENNING, Th et al.Astronomy and astrophysics (Berlin. Print). 2012, Vol 538, issn 0004-6361, 538A74.1-538A4.15, 1Article

TURBULENCE IN WEAKLY IONIZED PROTOPLANETARY DISKSFLOCK, M; HENNING, Th; KLAHR, H et al.The Astrophysical journal. 2012, Vol 761, Num 2, issn 0004-637X, 95.1-95.8, 1Article

CAN NEUTRAL AND IONIZED POLYCYCLIC AROMATIC HYDROCARBONS BE CARRIERS OF THE ULTRAVIOLET EXTINCTION BUMP AND THE DIFFUSE INTERSTELLAR BANDS?STEGLICH, M; BOUWMAN, J; HUISKEN, F et al.The Astrophysical journal. 2011, Vol 742, Num 1, issn 0004-637X, 2.1-2.12, 1Article

Do we need to know the temperature in prestellar cores?PAVLYUCHENKOV, Ya; HENNING, Th; WIEBE, D et al.The Astrophysical journal. 2007, Vol 669, Num 2, issn 0004-637X, L101-L104, 2Article

VLT/NACO adaptive optics imaging of GSS 30 IRS1 : a protostellar binary system?CHEN, X. P; LAUNHARDT, R; HENNING, Th et al.Astronomy and astrophysics (Berlin. Print). 2007, Vol 475, Num 1, pp 277-280, issn 0004-6361, 4 p.Article

Gravoturbulent formation of planetesimalsJOHANSEN, A; KLAHR, H; HENNING, Th et al.The Astrophysical journal. 2006, Vol 636, Num 2, pp 1121-1134, issn 0004-637X, 14 p., 1Article

On the stability of radiation-pressure-dominated cavitiesKUIPER, R; KLAHR, H; BEUTHER, H et al.Astronomy and astrophysics (Berlin. Print). 2012, Vol 537, issn 0004-6361, 537A122.1-537A122.13, 2Article

Dust rings and filaments around the isolated young star V1331 CygniQUANZ, S. P; APAI, D; HENNING, Th et al.The Astrophysical journal. 2007, Vol 656, Num 1, pp 287-292, issn 0004-637X, 6 p., 1Article

New Herbig-Haro objects in the L1617 and L1646 dark cloudsWANG, H; STECKLUM, B; HENNING, Th et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 437, Num 1, pp 169-175, issn 0004-6361, 7 p.Article

Synthetic observations of first hydrostatic cores in collapsing low-mass dense cores I. Spectral energy distributions and evolutionary sequenceCOMMERCON, B; LAUNHARDT, R; DULLEMOND, C et al.Astronomy and astrophysics (Berlin. Print). 2012, Vol 545, issn 0004-6361, A98.1-A98.12, 2Article

A highly efficient measure of mass segregation in star clustersOJCZAK, C; SPURZEM, R; HENNING, Th et al.Astronomy and astrophysics (Berlin. Print). 2011, Vol 532, issn 0004-6361, A119.1-A119.11, 2Article

Coagulation, fragmentation and radial motion of solid particles in protoplanetary disksBRAUER, F; DULLEMOND, C. P; HENNING, Th et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 480, Num 3, pp 859-877, issn 0004-6361, 19 p.Article

A rotating disk around the very young massive star AFGL 490'SCHREYER, K; SEMENOV, D; HENNING, Th et al.The Astrophysical journal. 2006, Vol 637, Num 2, issn 0004-637X, L129-L132, 2Article

Modelling the optical properties of composite and porous interstellar grainsVOSHCHINNIKOV, N. V; II'IN, V. B; HENNING, Th et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 429, Num 2, pp 371-381, issn 0004-6361, 11 p.Article

Infrared spectroscopy of calcium-aluminium-rich inclusions : Analog material for protoplanetary dust?POSCH, Th; MUTSCHKE, H; TRIELOFF, M et al.The Astrophysical journal. 2007, Vol 656, Num 1, pp 615-620, issn 0004-637X, 6 p., 1Article

The low-mass initial mass function of the field population in the Large Magellanic Cloud with Hubble Space Telescope WFPC2 observationsGOULIERMIS, D; BRANDNER, W; HENNING, Th et al.The Astrophysical journal. 2006, Vol 641, Num 2, pp 838-851, issn 0004-637X, 14 p., 1Article

Disk-disk encounters between low-mass protoplanetary accretion disksPFALZNER, S; UMBREIT, S; HENNING, Th et al.The Astrophysical journal. 2005, Vol 629, Num 1, pp 526-534, issn 0004-637X, 9 p., 1Article

Infrared portrait of the nearby massive star-forming region IRAS 09002-4732APAI, D; LINZ, H; HENNING, Th et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 434, Num 3, pp 987-1003, issn 0004-6361, 17 p.Article

Reduction of chemical networks. II. Analysis of the fractional ionisation in protoplanetary discsSEMENOV, D; WIEBE, D; HENNING, Th et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 417, Num 1, pp 93-106, issn 0004-6361, 14 p.Article

Mass segregation and elongation of the starburst cluster Westerlund 1GENNARO, M; BRANDNER, W; STOLTE, A et al.Monthly notices of the Royal Astronomical Society (Print). 2011, Vol 412, Num 4, pp 2469-2488, issn 0035-8711, 20 p.Article

Planetesimal formation near the snow line in MRI-driven turbulent protoplanetary disksBRAUER, F; HENNING, Th; DULLEMOND, C. P et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 487, Num 1, issn 0004-6361, L1-L4Article

SPECTRAL PROPERTIES OF GAS-PHASE CONDENSED FULLERENE-LIKE CARBON NANOPARTICLES FROM FAR-ULTRAVIOLET TO INFRARED WAVELENGTHSJÄGER, C; MUTSCHKE, H; HENNING, Th et al.The Astrophysical journal. 2008, Vol 689, Num 1, pp 249-259, issn 0004-637X, 11 p., 1Article