2020A&A...642A.222H


Query : 2020A&A...642A.222H

2020A&A...642A.222H - Astronomy and Astrophysics, volume 642A, 222-222 (2020/10-1)

Sulphur and carbon isotopes towards Galactic centre clouds.

HUMIRE P.K., THIEL V., HENKEL C., BELLOCHE A., LOISON J.-C., PILLAI T., RIQUELME D., WAKELAM V., LANGER N., HERNANDEZ-GOMEZ A., MAUERSBERGER R. and MENTEN K.M.

Abstract (from CDS):


Context. Measuring isotopic ratios is a sensitive technique used to obtain information on stellar nucleosynthesis and chemical evolution.
Aims. We present measurements of the carbon and sulphur abundances in the interstellar medium of the central region of our Galaxy. The selected targets are the +50km/s Cloud and several line-of-sight clouds towards Sgr B2(N).
Methods. Towards the +50km/s Cloud, we observed the J=2-1 rotational transitions of 12C32S, 12C34S, 13C32S, 12C33S, and 13C34S, and the J=3-2 transitions of 12C32S and 12C34S with the IRAM-30m telescope, as well as the J=6-5 transitions of 12C34S and 13C32S with the APEX 12m telescope, all in emission. The J=2-1 rotational transitions of 12C32S, 12C34S, 13C32S, and 13C34S were observed with ALMA in the envelope of Sgr B2(N), with those of 12C32S and 12C34S also observed in the line-of-sight clouds towards Sgr B2(N), all in absorption.
Results. In the +50km/s Cloud we derive a 12C/13C isotopic ratio of 22.1–2.4+3.3, that leads, with the measured 13C32S/12C34S line intensity ratio, to a 32S/34S ratio of 16.3–2.4+3.0. We also derive the 32S/34S isotopic ratio more directly from the two isotopologues 13C32S and 13C34S, which leads to an independent 32S/34S estimation of 16.3–1.7+2.1 and 17.9±5.0 for the +50km/s Cloud and Sgr B2(N), respectively. We also obtain a 34S/33S ratio of 4.3±0.2 in the +50km/s Cloud.
Conclusions. Previous studies observed a decreasing trend in the 32S/34S isotopic ratios when approaching the Galactic centre. Our result indicates a termination of this tendency at least at a galactocentric distance of 130–30+60_pc. This is at variance with findings based on 12C/13C, 14N/15N, and 18O/17O isotope ratios, where the above-mentioned trend is observed to continue right to the central molecular zone. This can indicate a drop in the production of massive stars at the Galactic centre, in the same line as recent metallicity gradient ([Fe/H]) studies, and opens the work towards a comparison with Galactic and stellar evolution models.

Abstract Copyright: © P. K. Humire et al. 2020

Journal keyword(s): Galaxy: centre - submillimetre: ISM - Galaxy: formation - Galaxy: evolution - stars: atmospheres - submillimetre: general

VizieR on-line data: <Available at CDS (J/A+A/642/A222): table1.dat 50cloud/*_f.dat 50cloud/*-?.dat sgrb2_n/*>

Simbad objects: 19

goto Full paper

goto View the references in ADS

Number of rows : 19
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 NGC 253 SyG 00 47 33.134 -25 17 19.68   8.03   6.94 8.1 ~ 3336 2
2 LDN 1544 DNe 05 04 16.6 +25 10 48           ~ 863 0
3 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 17434 0
4 LHA 120-N 159 HII 05 39 46.650 -69 45 39.94           ~ 276 2
5 NGC 4945 Sy2 13 05 27.279 -49 28 04.44   9.31 14.40 7.55   ~ 1475 2
6 NAME Sgr A Region reg 17 45 12 -28 48.3           ~ 939 0
7 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 14416 0
8 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 4391 3
9 0FGL J1746.0-2900 gam 17 45 41 -29 00.8           ~ 493 2
10 GCM -0.02 -0.07 MoC 17 45 50.4 -28 59 06           ~ 164 0
11 NAME Sgr B MoC 17 47 02 -28 25.4           ~ 223 0
12 [QSR2011] Sgr B2(N)-SMA2 cor 17 47 19.885 -28 22 13.29           ~ 93 0
13 [BMG2016] Sgr B2(N1) cor 17 47 19.889 -28 22 18.22           ~ 57 0
14 NAME Sgr B2 HII K4 HII 17 47 20.00 -28 22 04.8           ~ 18 0
15 [BMG2016] Sgr B2(N5) cor 17 47 20.047 -28 22 41.34           ~ 20 0
16 NAME Sgr B2 (North) Rad 17 47 20.2 -28 22 21           ~ 673 1
17 NAME Sgr B2 HII K5 HII 17 47 20.3 -28 22 13           ~ 15 0
18 NAME Sgr B2 HII K6 HII 17 47 20.36 -28 22 12.1           ~ 14 0
19 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 2266 1

To bookmark this query, right click on this link: simbad:objects in 2020A&A...642A.222H and select 'bookmark this link' or equivalent in the popup menu