THE 3 RINGS OF THE ISOLATED GALAXY NGC-7217

Citation
L. Verdesmontenegro et al., THE 3 RINGS OF THE ISOLATED GALAXY NGC-7217, Astronomy and astrophysics, 300(1), 1995, pp. 65-77
Citations number
31
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00046361
Volume
300
Issue
1
Year of publication
1995
Pages
65 - 77
Database
ISI
SICI code
0004-6361(1995)300:1<65:T3ROTI>2.0.ZU;2-Z
Abstract
We present WSRT HI line observations, together with CCD-BVRI photometr y, of NGC 7217, which is known to be an isolated galaxy with an inner ring, an inner pseudoring and an outer ring, but for which no clear bi -symmetric distortion is immeadiately apparent. Assuming, as is known to be the case for barred galaxies, that the outer ring corresponds to the outer Lindblad resonance, we have derived the expected locations for the other resonances using a combined optical/H I rotation curve. Our result is that the observed inner ring coincides with the inner Li ndblad resonance and the inner pseudoring with the ultraharmonic (4:1) resonance. The associated pattern speed is 86.0 km s(-1) kpc(-1) Howe ver, it is less clear which feature is actually setting up this patter n. The outer ring, which has a size of similar or equal to 6.3 x 5.9 k pc, contains roughly two-thirds of the total H I mass, and has bluer c olours and more intense Her emission than the main disk. A Fourier ana lysis of the B - I colour along this ring suggests that it is composed of 9 blobs, indicating the existence of a bead instability. This is i n agreement with a simple calculation showing that the number of Jeans lengths along the ring is also 9, and that self-gravity is probably i mportant here. Clumps also exist in the inner pseudoring, but they are less well defined, and there is no HI concentration along it. This ri ng has redder colours than the outer ring. The blue inner ring is inco mplete, coincides with a complete and intense Ha ring, and is surround ed by a redder ring. A spiral-like structure extends from the inner ri ng out to the inner pseudoring, with the same winding direction as the outer flocculent arms. We have constructed a mass model, from which w e obtain a mass-to-I-band luminosity ratio of 5.1 for the bulge, and 1 .8 for the disk. The core radius of the halo is 11.0 kpc, and its cent ral density 0.062 Mo pc(-3). The ratio of halo core radius to optical radius is thus of order unity.