Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-12-03
Astronomy and Astrophysics
Astrophysics
16 pages, 7 figures, uses mn.sty, to appear in MNRAS
Scientific paper
10.1046/j.1365-8711.1999.02380.x
ISO-SWS spectroscopy of the WR galaxy NGC5253 is presented, and analysed to provide estimates of its hot young star population. Our approach differs from previous investigations in that we are able to distinguish between the regions in which different infrared fine-structure lines form, using complementary ground-based observations. The high excitation nebular [SIV] emission is formed in a very compact region, which we attribute to the central super-star-nucleus, and lower excitation [NeII] nebular emission originates in the galactic core. We use photo-ionization modelling coupled with the latest theoretical O-star flux distributions to derive effective stellar temperatures and ionization parameters of Teff>38kK, logQ=8.25 for the compact nucleus, with Teff=35kK, logQ<8 for the larger core. Results are supported by more sophisticated calculations using evolutionary synthesis models. We assess the contribution that Wolf-Rayet stars may make to highly ionized nebular lines (e.g. [OIV]). From our Br(alpha) flux, the 2" nucleus contains the equivalent of approximately 1000 O7V star equivalents and the starburst there is 2-3Myr old; the 20" core contains about 2500 O7V star equivalents, with a representative age of 5Myr. The Lyman ionizing flux of the nucleus is equivalent to the 30 Doradus region. These quantities are in good agreement with the observed mid-IR dust luminosity of 7.8x10^8 L(sun) Since this structure of hot clusters embedded in cooler emission may be common in dwarf starbursts, observing a galaxy solely with a large aperture may result in confusion. Neglecting the spatial distribution of nebular emission in NGC5253, implies `global' stellar temperatures (or ages) of 36kK (4.8Myr) and 39kK (2.9 or 4.4Myr) from the observed [NeIII/II] and [SIV/III] line ratios, assuming logQ=8.
Beck Sara C.
Conti Peter S.
Crowther Paul A.
Morris Pat W.
Sutherland Ralph S.
No associations
LandOfFree
Properties of Hot Stars in the Wolf-Rayet galaxy NGC5253 from ISO Spectroscopy does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Properties of Hot Stars in the Wolf-Rayet galaxy NGC5253 from ISO Spectroscopy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Properties of Hot Stars in the Wolf-Rayet galaxy NGC5253 from ISO Spectroscopy will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-208298