activity
19972015
most citedSimulations of Normal Spiral Galaxies

76 citations · 248 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2015★ 34 cited

The distribution of dark and luminous matter inferred from extended rotation curves

Roelof Bottema, Jose Luis G. Pestana

A better understanding of the formation of mass structures in the universe can be obtained by determining the amount and distribution of dark and luminous matter in spiral galaxies…

astro-ph2003★ 76 cited

Simulations of Normal Spiral Galaxies

Roelof Bottema

Results are presented of numerical simulations of normal isolated late type spiral galaxies. Specifically the galaxy NGC 628 is used as a template. The method employs a TREESPH cod…

astro-ph2002★ 60 cited

MOND rotation curves for spiral galaxies with Cepheid-based distances

Roelof Bottema, Jose L. G. Pestana, Barry Rothberg +1

Rotation curves for four spiral galaxies with recently determined Cepheid-based distances are reconsidered in terms of modified Newtonian dynamics (MOND). For two of the objects, N…

astro-ph2002★ 11 cited

Dark and luminous matter in the NGC 3992 group of galaxies, II. The dwarf companions UGC 6923, UGC 6940, UGC 6969, and the Tully-Fisher relation

Roelof Bottema

Detailed neutral hydrogen observations have been obtained of the large barred spiral galaxy NGC 3992 and its three small companion spiral galaxies, UGC 6923, UGC 6940, and UGC 6969…

astro-ph2002★ 20 cited

Dark and luminous matter in the NGC 3992 group of galaxies, I. The large barred spiral NGC 3992

Roelof Bottema, Marc A. W. Verheijen

Detailed neutral hydrogen observations have been obtained of the large barred spiral galaxy NGC 3992 and its three small companion galaxies, UGC 6923, UGC 6940, and UGC 6969. For t…

astro-ph1999★ 1 cited

The kinematics of the bulge and the disc of NGC 7331

Roelof Bottema

Presented are spectroscopic emission and absorption line observations along the major axis of the Sb galaxy NGC 7331. The kinematics of the ionized gas and the stars appears to be…