2001MNRAS.327..385S


Query : 2001MNRAS.327..385S

2001MNRAS.327..385S - Mon. Not. R. Astron. Soc., 327, 385-396 (2001/October-3)

The energetics and mass loss of the dwarf starburst Markarian 33.

SUMMERS L.K., STEVENS I.R. and STRICKLAND D.K.

Abstract (from CDS):

We present ROSAT HRI X-ray data and optical imaging of the important dwarf starburst Markarian 33. We find an extended, complex, shell-like morphology in the X-ray emission, with an extent of ∼2.3.1.9kpc2,coincident with the right star-forming regions at the centre of the galaxy. The physical extent of this X-ray emission from Mrk 33 is very similar to the observed Hα emission, and suggests that the bulk of the X-ray emission is coming from an expanding superbubble.

We estimate the age and mass of Mrk 33's starburst to be 5.8Myr and 6.9.106Msolar respectively, with the energy injection rate in the central regions of the galaxy being ∼1041ergs–1, while the associated mass-loss rate from the star-forming regions is estimated to be ∼0.2M☉yr–1. We suggest that the X-ray emission is predominantly powered by starburst-type activity, and argue that a blow-out in the form of a galactic wind is the most likely fate for Mrk 33, resulting in the loss of most of the galaxy's metal-enriched material and a small fraction (<1 per cent) of the ISM.


Abstract Copyright: The Royal Astronomical Society

Journal keyword(s): stars: Wolf-Rayet - ISM: jets and outflows - galaxies: individual: Mrk 33 - galaxies: starburst - galaxies: stellar content - X-rays: galaxies

Nomenclature: Fig.2: [SSS2001] Mrk 33 W (Nos N, S). Fig.1, Table A1: [SSS2001] X-NN (Nos X-1 to X-23).

Simbad objects: 30

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Number of rows : 30
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 253 SyG 00 47 33.134 -25 17 19.68   8.03   6.94 8.1 ~ 3588 2
2 NGC 1569 rG 04 30 49.186 +64 50 52.52 11.72 11.86 11.03     ~ 1297 3
3 MCG-04-21-005 AGN 08 36 15.190 -26 24 33.66 12.04 11.93 11.45 11.09 12.3 ~ 600 3
4 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
5 SDSS J103102.05+542353.6 QSO 10 31 02.055 +54 23 53.64           ~ 6 0
6 SDSS J103130.32+542100.8 QSO 10 31 30.3178978032 +54 21 00.846269352           ~ 9 0
7 RX J103136.1+541843 X 10 31 36.1 +54 18 43           ~ 1 0
8 RX J103151.8+542518 X 10 31 51.8 +54 25 18           ~ 1 0
9 SDSS J103152.03+541727.6 QSO 10 31 52.0210986384 +54 17 27.686330808           ~ 7 0
10 RX J103153.1+541724 X 10 31 53.1 +54 17 24           ~ 1 0
11 RX J103155.4+541702 X 10 31 55.4 +54 17 02           ~ 1 0
12 RX J103156.6+543036 X 10 31 56.6 +54 30 36           ~ 1 0
13 RX J103205.5+543726 X 10 32 05.5 +54 37 26           ~ 1 0
14 RX J103209.1+543013 X 10 32 09.1 +54 30 13           ~ 1 0
15 RX J103219.4+541234 X 10 32 19.4 +54 12 34           ~ 1 0
16 RX J103219.5+543806 X 10 32 19.5 +54 38 06           ~ 1 0
17 RX J103229.2+542124 X 10 32 29.2 +54 21 24           ~ 1 0
18 [SSS2001] Mrk 33 N X 10 32 31.8 +54 24 04           ~ 2 0
19 [SSS2001] Mrk 33 S X 10 32 31.9 +54 24 03           ~ 2 0
20 Z 266-55 AGN 10 32 31.956 +54 24 03.53 13.29 13.66 13.13 12.71 12.27 ~ 381 1
21 RX J103233.6+542621 X 10 32 33.6 +54 26 21           ~ 1 0
22 RX J103244.0+543606 X 10 32 44.0 +54 36 06           ~ 1 0
23 RX J103249.0+543409 X 10 32 49.0 +54 34 09           ~ 1 0
24 RX J103249.3+541244 X 10 32 49.3 +54 12 44           ~ 1 0
25 RX J103251.5+541837 X 10 32 51.5 +54 18 37           ~ 1 0
26 RX J103322.8+542523 X 10 33 22.8 +54 25 23           ~ 1 0
27 RX J103341.9+541755 X 10 33 41.9 +54 17 55           ~ 1 0
28 RX J103349.7+541535 X 10 33 49.7 +54 15 35           ~ 1 0
29 RX J103402.6+543019 X 10 34 02.6 +54 30 19           ~ 1 0
30 NGC 5253 rG 13 39 55.990 -31 38 24.11 11.48 10.94 10.49 10.33 13.47 ~ 1421 4

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