2001A&A...372..833F


Query : 2001A&A...372..833F

2001A&A...372..833F - Astronomy and Astrophysics, volume 372, 833-850 (2001/6-4)

Kinematics of young stars. II. Galactic spiral structure.

FERNANDEZ D., FIGUERAS F. and TORRA J.

Abstract (from CDS):

The young star velocity field is analysed by means of a galactic model which takes into account solar motion, differential galactic rotation and spiral arm kinematics. We use two samples of Hipparcos data, one containing O- and B-type stars and another one composed of Cepheid variable stars. The robustness of our method is tested through careful kinematic simulations. Our results show a galactic rotation curve with a classical value of A Oort constant for the O and B star sample (AOB=13.7-13.8km/s/kpc) and a higher value for Cepheids (ACep=14.9-16.9km/s/kpc, depending on the cosmic distance scale chosen). The second-order term is found to be small, compatible with a zero value. The study of the residuals shows the need for a K-term up to a heliocentric distance of 4kpc, obtaining a value K=-(1-3)km/s/kpc. The results obtained for the spiral structure from O and B stars and Cepheids show good agreement. The Sun is located relatively near the minimum of the spiral perturbation potential (ψ=284-20°) and very near the corotation circle. The angular rotation velocity of the spiral pattern was found to be Ωp≃30km/s/kpc.

Abstract Copyright:

Journal keyword(s): Galaxy: kinematics and dynamics - Galaxy: solar neighbourhood - Galaxy: structure - stars: early-type - stars: kinematics - stars: variables: Cepheids

Simbad objects: 7

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Number of rows : 7
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 NGC 869 OpC 02 18 58 +57 08.0           ~ 456 0
2 Ass Per OB 1 As* 02 21 +57.6           ~ 166 1
3 NGC 884 OpC 02 22 20 +57 08.9           ~ 467 0
4 Ass Cas OB 6 As* 02 43 +61.3           ~ 121 0
5 Ass Sgr OB 1 As* 18 06 -22.8           ~ 123 0
6 Ass Ser OB 1 As* 18 21 -14.4           ~ 74 0
7 Ass Sct OB 2 As* 18 35 -08.9           ~ 37 0

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2022.08.18-03:30:55

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