Ripples in disk galaxies
Journal Article
·
· Astrophys. J.; (United States)
Evidence is presented that ripples occur not only in ellipticals but also in disk galaxies of Hubble types S0, S0/Sa, and Sa, and probably even in the Sbc galaxy NGC 3310. It is argued that the ripples cannot usually have resulted from transient spiral waves or other forced vibrations in existing disks, but instead consist of extraneous sheetlike matter. The frequent presence of major disk-shaped companions suggests that ripple material may be acquired not only through wholesale mergers but also through mass transfer from neighbor galaxies. The implications of ripples in early-type disk galaxies are addressed. 40 references.
- Research Organization:
- Carnegie Institution of Washington, DC (USA); Kitt Peak National Observatory, Tucson, AZ (USA)
- OSTI ID:
- 7188436
- Journal Information:
- Astrophys. J.; (United States), Vol. 328
- Country of Publication:
- United States
- Language:
- English
Similar Records
A REVISED PARALLEL-SEQUENCE MORPHOLOGICAL CLASSIFICATION OF GALAXIES: STRUCTURE AND FORMATION OF S0 AND SPHEROIDAL GALAXIES
THE OUTER DISKS OF EARLY-TYPE GALAXIES. II. SURFACE-BRIGHTNESS PROFILES OF UNBARRED GALAXIES AND TRENDS WITH HUBBLE TYPE
GALAXY-SCALE STAR FORMATION ON THE RED SEQUENCE: THE CONTINUED GROWTH OF S0s AND THE QUIESCENCE OF ELLIPTICALS
Journal Article
·
Sun Jan 01 00:00:00 EST 2012
· Astrophysical Journal, Supplement Series
·
OSTI ID:7188436
THE OUTER DISKS OF EARLY-TYPE GALAXIES. II. SURFACE-BRIGHTNESS PROFILES OF UNBARRED GALAXIES AND TRENDS WITH HUBBLE TYPE
Journal Article
·
Tue Nov 15 00:00:00 EST 2011
· Astronomical Journal (New York, N.Y. Online)
·
OSTI ID:7188436
GALAXY-SCALE STAR FORMATION ON THE RED SEQUENCE: THE CONTINUED GROWTH OF S0s AND THE QUIESCENCE OF ELLIPTICALS
Journal Article
·
Mon Aug 20 00:00:00 EDT 2012
· Astrophysical Journal
·
OSTI ID:7188436
+1 more