Age, evolution, and dispersion of the loose groups of blue stars in the northeast radio lobe of Centaurus A

Citation
Ci. Fassett et Ja. Graham, Age, evolution, and dispersion of the loose groups of blue stars in the northeast radio lobe of Centaurus A, ASTROPHYS J, 538(2), 2000, pp. 594-607
Citations number
26
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
538
Issue
2
Year of publication
2000
Part
1
Pages
594 - 607
Database
ISI
SICI code
0004-637X(20000801)538:2<594:AEADOT>2.0.ZU;2-P
Abstract
The association of shocked gas and loose groups of young stars in the north east radio lobe of Centaurus A (NGC 5128) provides direct evidence for shoc k-induced star formation. In this paper, we present UBV photometry of the b lue stars based on observations made with the 2.5 m du Pont Telescope at La s Campanas Observatory. In a held covering 8.'8 x 8.'8, three groups are id entified. Color-magnitude and color-color diagrams are plotted for each gro up. Two-color photometry of the many foreground held stars belonging to our own Galaxy indicates a foreground reddening EB-V = 0.14 mag +/- 0.02 mag. The new photometry is compared with that carried out in a small section of the field with the Hubble Space Telescope. The HST frames, in conjunction w ith the ground-based material allow compact star clusters to be identified, some of which are exciting small H II regions. Positions, finding charts, and photometry are given for 50 stars with V < 23.0 mag and (B-V)< 0.4 mag. The brightest blue star, at V = 19.94 mag, has an estimated absolute visua l magnitude M-V = -8.2 mag, which is comparable to that of the brightest A- type supergiants in the Large Magellanic Cloud. Most of the blue stars lie just inside the 1.4 GHz contours of the large-scale jetlike feature recentl y detected by Morganti et al. It is suggested that rather than being a comp onent of the jet that powers the radio lobes, this feature, which resembles a spiral arm of a normal galaxy, results from compression of ambient gas b y the jet. Bolometric magnitudes and effective temperatures are derived for the bright blue stars and plotted. Isochrones based on the Geneva evolutio nary tracks are fitted and indicate a significant age spread for the stars extending up to 15 million years. The older stars are distributed more wide ly than the younger stars indicating that star formation extends over time and that the blue stars eventually disperse into the extended stellar envel ope of the galaxy.