249 citations · 515 across the 12 of their papers we have counts for
12 papers
Kinematics of the Local Universe XIV. Measurements from the 21 cm line and the HI mass function from a homogeneous catalog gathered with the Nançay radio telescope
Gilles Theureau, Nicole Coudreau, Nicole Hallet +2
This paper presents 828 new 21 cm neutral hydrogen line measurements carried out with the FORT receiver of the meridian transit Nançay radio telescope (NRT) in the years 2000 -- 20…
Revisiting the optical depth of spiral galaxies using the Tully-Fisher B relation
E. Kankare, M. Hanski, G. Theureau +1
Aims. We attempt to determine the optical depth of spiral galaxy disks by a statistical study of new Tully-Fisher data from the ongoing KLUN+ survey, and to clarify the difference…
Kinematics of the Local Universe XIII. 21-cm line measurements of 452 galaxies with the Nançay radiotelescope, JHK Tully-Fisher relation and preliminary maps of the peculiar velocity field
Gilles Theureau, Mikko Hanski, Nicole Coudreau +2
This paper presents 452 new 21-cm neutral hydrogen line measurements carried out with the FORT receiver of the meridian transit Nançay radiotelescope (NRT) in the period April 2003…
Calibration of the distance scale from galactic Cepheids:II Use of the HIPPARCOS calibration
G. Paturel, P. Teerikorpi, G. Theureau +3
New estimate of the distances of 36 nearby galaxies is presented. It is based on the calibration of the V- and I-band Period-Lumi- nosity relations for galactic Cepheids measured b…
Calibration of the distance scale from galactic Cepheids: I Calibration based on the GFG sample
G. Paturel, G. Theureau, P. Fouque +3
New estimates of the distances of 36 nearby galaxies are presented based on accurate distances of galactic Cepheids obtained by Gieren, Fouque and Gomez (1998) from the geometrical…
Kinematics of the local universe IX. The Perseus-Pisces supercluster and the Tolman-Bondi model
Mikko Hanski, Gilles Theureau, Timo Ekholm +1
We study the mass distribution and the infall pattern of the Perseus-Pisces (PP) supercluster. First we calculate the mass of the central part of PP, a sphere with a radius of 15/h…