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- Mon. Not. R. Astron. Soc. 319, 377392 (2000) N-body model for M51 I. Multiple encounter versus single passage?
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- Mon. Not. R. Astron. Soc. 383, 317329 (2008) doi:10.1111/j.1365-2966.2007.12548.x Comparison of bar strengths in optical and near-infrared for the
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- 3XEOLFDWLRQ RI WKH $FDGHP\ RI )LQODQG (9$/8$7,21 2) ),11,6+ $6752120<
- Icarus 173 (2005) 508521 www.elsevier.com/locate/icarus
- Icarus 172 (2004) 328348 www.elsevier.com/locate/icarus
- ASTRONOMY & ASTROPHYSICS MAY I 1998, PAGE 517 SUPPLEMENT SERIES
- The Astronomical Journal, 136:300311, 2008 July doi:10.1088/0004-6256/136/1/300 c 2008. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- A&A 405, 3152 (2003) DOI: 10.1051/0004-6361:20030542
- Icarus 177 (2005) 3262 www.elsevier.com/locate/icarus
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- THE ASTRONOMICAL JOURNAL, 117:792810, 1999 February 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
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- Mon. Not. R. Astron. Soc. 337, 12331244 (2002) Simulations of central structure in barred galaxies
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- Icarus 170 (2004) 7090 www.elsevier.com/locate/icarus
- Icarus 167 (2004) 330346 www.elsevier.com/locate/icarus
- Mon. Not. R. Astron. Soc. 362, 13191347 (2005) doi:10.1111/j.1365-2966.2005.09404.x Multicomponent decompositions for a sample of S0 galaxies
- Icarus 189 (2007) 493522 www.elsevier.com/locate/icarus
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- The Astrophysical Journal, 692:L34L39, 2009 February 10 doi:10.1088/0004-637X/692/1/L34 c 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- ASTRONOMY & ASTROPHYSICS JANUARY I 2000, PAGE 103 SUPPLEMENT SERIES
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- Mon. Not. R. Astron. Soc. 319, 393413 (2000) N-body model for M51 II. Inner structure
- This article appeared in a journal published by Elsevier. The attached copy is furnished to the author for internal non-commercial research
- The Astronomical Journal, 136:980993, 2008 September doi:10.1088/0004-6256/136/3/980 c 2008. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- Mon. Not. R. Astron. Soc. 388, 18031818 (2008) doi:10.1111/j.1365-2966.2008.13522.x Model-based pattern speed estimates for 38 barred galaxies
- Mon. Not. R. Astron. Soc. 381, 401417 (2007) doi:10.1111/j.1365-2966.2007.12299.x Properties of bars and bulges in the Hubble sequence
- A&A 466, 847854 (2007) DOI: 10.1051/0004-6361:20077071
- arXiv:astro-ph/0305530v128May2003 Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 3 January 2004 (MN LATEX style file v2.2)
- COMPARISON OF BAR STRENGTHS AND FRACTIONS OF BARS IN ACTIVE AND NONACTIVE GALAXIES
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- SELF-GRAVITY WAKE STRUCTURES IN SATURN'S A RING REVEALED BY CASSINI VIMS Matthew M. Hedman and Philip D. Nicholson
- Icarus 189 (2007) 523537 www.elsevier.com/locate/icarus
- Structures induced by small moonlets in Saturn's rings: Implications for the Cassini Mission
- The Astrophysical Journal, 631:L129L132, 2005 October 1 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- Mon. Not. R. Astron. Soc. 337, 11181138 (2002) Bar strengths in spiral galaxies estimated from 2MASS images
- Astron. Astrophys. 362, 465586 (2000) ASTROPHYSICS
- Astron. Astrophys. 348, 737754 (1999) ASTROPHYSICS
- arXiv:astro-ph/0312535v119Dec2003 Astronomy & Astrophysics manuscript no. ifc001 January 2, 2004 (DOI: will be inserted by hand later)
- Hindawi Publishing Corporation Advances in Astronomy
- Mon. Not. R. Astron. Soc. 418, 14521490 (2011) doi:10.1111/j.1365-2966.2011.19283.x Near-infrared atlas of S0-Sa galaxies (NIRS0S)
- Mon. Not. R. Astron. Soc. 405, 10891118 (2010) doi:10.1111/j.1365-2966.2010.16521.x Photometric scaling relations of lenticular and spiral galaxies
- DOI: 10.1126/science.1205672 , 672 (2011);332Science
- N-body simulations of viscous instability of planetary rings Heikki Salo a,*, Jrgen Schmidt b
- The Astrophysical Journal Letters, 715:L56L61, 2010 May 20 doi:10.1088/2041-8205/715/1/L56 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- The Astrophysical Journal Letters, 745:L24 (6pp), 2012 February 1 doi:10.1088/2041-8205/745/2/L24 C 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A.