1999A&A...351..442S

Query : 1999A&A...351..442S

1999A&A...351..442S - Astronomy and Astrophysics, volume 351442-446 (1999/11-2)

Maximal halos in high-luminosity spiral galaxies.

SALUCCI P. and PERSIC M.

Abstract (from CDS):

We test the halo dominated mass model, recently proposed for high-luminosity galaxies, against the rotation velocity data of a large sample of L ∼L* spirals. We find that this model does not reproduce the general kinematic properties required. The alternative disc dominated model, on the contrary, easily fits the data.

Abstract Copyright: ∼

Journal keyword(s): galaxies: kinematics and dynamics - galaxies: spiral - galaxies: structure - cosmology: dark matter

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NGC 2179 Sy2 06 08 02.2326823704 -21 44 48.266982276   13.33 12.45 11.58   ~ 66 0
2 NGC 2775 AG? 09 10 20.1334093488 +07 02 16.874157048   11.417 10.481 9.920 8.994 ~ 377 0
3 NGC 5033 Sy2 13 13 27.535 +36 35 37.14   11.01 12.03 9.73   ~ 909 1
4 M 63 LIN 13 15 49.2741893928 +42 01 45.728076108   9.34 8.59 8.35   ~ 1292 2

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