2012MNRAS.421.3399N


Query : 2012MNRAS.421.3399N

2012MNRAS.421.3399N - Mon. Not. R. Astron. Soc., 421, 3399-3408 (2012/April-3)

Exploring the effects of high-velocity flows in abundance determinations in H II regions: bidimensional spectroscopy of HH 204 in the Orion nebula.

NUNEZ-DIAZ M., MESA-DELGADO A., ESTEBAN C., LOPEZ-MARTIN L., GARCIA-ROJAS J. and LURIDIANA V.

Abstract (from CDS):

We present results from integral field optical spectroscopy with the Potsdam Multi-Aperture Spectrograph of the Herbig–Haro (HH) object HH 204, with a spatial sampling of 1 {x} 1 arcsec2. We have obtained maps of different emission lines, physical conditions and ionic abundances from collisionally excited lines. The ionization structure of the object indicates that the head of the bow shock is optically thick and has developed a trapped ionization front. The density at the head is at least five times larger than in the background ionized gas. We discover a narrow arc of high Te([N II]) values delineating the southeast edge of the head. The temperature in this zone is about 1000 K higher than in the rest of the field and should correspond to a shock-heated zone at the leading working surface of the gas flow. This is the first time this kind of feature is observed in a photoionized HH object. We find that the O+ and O abundance maps show anomalous values at separate areas of the bow shock probably due to: (a) overestimation of the collisional de-excitation effects of the [O II] lines in the compressed gas at the head of the bow shock, and (b) the use of a too high Te([N II]) at the area of the leading working surface of the flow.

Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): ISM: abundances - H {sc ii} regions - Herbig - Haro objects - ISM: individual objects: HH 204 - ISM: individual objects: Orion nebula - ISM: jets and outflows

Simbad objects: 18

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Number of rows : 18
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 BD+52 913 WD* 05 05 30.6180977592 +52 49 51.919301604 10.25 11.44 11.69 11.93 12.108 DA.8 1153 0
2 HH 505 HH 05 34 40.8 -05 22 39           ~ 14 1
3 NAME Orion Nebula Cluster OpC 05 35.0 -05 29           ~ 2514 0
4 HH 202 HH 05 35 11.468 -05 22 46.34           ~ 74 4
5 NAME Orion-KL SFR 05 35 14.16 -05 22 21.5           ~ 2421 1
6 * tet01 Ori C SB* 05 35 16.4662967280 -05 23 22.921811880 4.20 5.15 5.13 4.91 4.73 O7Vp 1479 1
7 NAME Ori Trapezium OpC 05 35 16.5 -05 23 14           ~ 1708 1
8 M 42 HII 05 35 16.8 -05 23 15           ~ 4411 0
9 HH 529 HH 05 35.3 -05 23           ~ 38 4
10 HH 203 HH 05 35 22.225 -05 24 58.12           ~ 74 4
11 HH 204 HH 05 35 22.6 -05 25 13           ~ 84 4
12 * tet02 Ori A SB* 05 35 22.9012398264 -05 24 57.832632108 5.37 6.30 6.39 6.30 6.35 O9.5IVp 576 0
13 HH 1 HH 05 36 20.8 -06 45 13           ~ 415 1
14 LDN 1641 MoC 05 39.0 -07 00           ~ 502 0
15 Haro 5-27 TT* 05 39 39.8261592024 -02 31 21.865624536 14.589   14.30 13.92 13.073 K5.5 93 0
16 Feige 34 HS* 10 39 36.7358839104 +43 06 09.212615280 9.613 10.91 11.14 11.319 11.464 sdOp 731 0
17 Feige 110 HS* 23 19 58.3996844256 -05 09 56.171142864 10.360 11.45 11.50 11.970 12.145 sdO8VIIIHe5 673 1
18 NAME Orion's Veil HI ~ ~           ~ 63 0

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