Artigo Acesso aberto Revisado por pares

Tests of the Tully-Fisher Relation.II.Scatter Using Optical Rotation Curves

1997; Institute of Physics; Volume: 113; Linguagem: Inglês

10.1086/118416

ISSN

1538-3881

Autores

Somak Raychaudhury, Kaspar von Braun, G. M. Bernstein, Puragra Guhathakurta,

Tópico(s)

Statistical Mechanics and Entropy

Resumo

view Abstract Citations (23) References (11) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Tests of the Tully-Fisher Relation.II.Scatter Using Optical Rotation Curves Raychaudhury, Somak ; von Braun, Kaspar ; Bernstein, Gary M. ; Guhathakurta, Puragra Abstract We investigate the amount of scatter in the Tully-Fisher relation (TFR) when using optical long-slit \ha\ rotation curves to determine the velocity widths of spiral galaxies. We study a sample of 25 galaxies in the Coma region of the sky which were shown in Bernstein et al. \markcite{B1} (1994) to exhibit an extraordinarily low scatter of 0.10 mag RMS in the I magnitude vs 21-cm width TFR. Using the same I magnitudes with new widths derived from high-quality \ha\ rotation curves, we measure an RMS scatter of 0.14 mag in the TFR. This suggests that measurement errors and ``astrophysical errors'' (such as non-circular gas motion) on the \ha\ velocity widths are below 6%, and optical widths are nearly as good for TFR studies as 21-cm widths. The scatter and form of the TFR are found to be robust under choice of velocity width-extraction algorithm, as long as the central portions of the optical rotation curve are ignored and low-S/N points are not weighted too heavily. In this small sample there is no evidence that rotation curve shapes vary systematically with rotation velocity, nor that rotation curve shape can be used to reduce the scatter in the TFR. Publication: The Astronomical Journal Pub Date: June 1997 DOI: 10.1086/118416 arXiv: arXiv:astro-ph/9703168 Bibcode: 1997AJ....113.2046R Keywords: Astrophysics E-Print: 17 pages (including 2 tables and 5 Encapsulated Postscript figures), uses AAS LaTeX, to appear in Astronomical Journal, June 1997 issue full text sources arXiv | ADS | data products NED (26) SIMBAD (25) Related Materials (1) Part 1: 1994AJ....107.1962B

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