Circumnuclear star formation in M100

Citation
Sd. Ryder et Jh. Knapen, Circumnuclear star formation in M100, ASTRO SP SC, 276(2-4), 2001, pp. 405-412
Citations number
14
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICS AND SPACE SCIENCE
ISSN journal
0004640X → ACNP
Volume
276
Issue
2-4
Year of publication
2001
Pages
405 - 412
Database
ISI
SICI code
0004-640X(2001)276:2-4<405:CSFIM>2.0.ZU;2-F
Abstract
Near-infrared (JHK) images of the nucleus of the barred spiral galaxy M100 (NGC 4321) have been obtained using a high-bandwidth tip-tilt secondary and fast guider system on the 3.8 m United Kingdom Infrared Telescope (UKIRT). The resulting images, with a resolution of 0 " .34' at K, reveal for the f irst time a host of compact 'knots', which appear to be the result of a rec ent burst (or bursts) of star formation. Confirmation of this comes from K- band spectroscopy of these knots with CGS4 on UKIRT, which shows Br gamma e mission and CO absorption features. A comparison with starburst evolutionar y models suggests ages for these knots of between 17 and 27 Myr, and a stel lar population dominated by late-type supergiants.