2023A&A...670A.110N


Query : 2023A&A...670A.110N

2023A&A...670A.110N - Astronomy and Astrophysics, volume 670A110 (2023/2-1)

Linking the dust and chemical evolution: Taurus and Perseus New collisional rates for HCN, HNC, and their C, N, and H isotopologues.

NAVARRO-ALMAIDA D., BOP C.T., LIQUE F., ESPLUGUES G., RODRIGUEZ-BARAS M., KRAMER C., ROMERO C.E., FUENTE A., CASELLI P., RIVIERE-MARICHALAR P., KIRK J.M., CHACON-TANARRO A., ROUEFF E., MROCZKOWSKI T., BHANDARKAR T., DEVLIN M., DICKER S., LOWE I., MASON B., SARAZIN C.L. and SIEVERS J.

Abstract (from CDS):


Context. HCN, HNC, and their isotopologues are ubiquitous molecules that can serve as chemical thermometers and evolutionary tracers to characterize star-forming regions. Despite their importance in carrying information that is vital to studies of the chemistry and evolution of star-forming regions, the collision rates of some of these molecules have not been available for rigorous studies in the past.
Aims. Our goal is to perform an up-to-date gas and dust chemical characterization of two different star-forming regions, TMC 1-C and NGC 1333-C7, using new collisional rates of HCN, HNC, and their isotopologues. We investigated the possible effects of the environment and stellar feedback in their chemistry and their evolution.
Methods. We used updated collisional rates of HCN, HNC, and their isotopologues in our analysis of the chemistry of TMC 1-C (Taurus) and NGC 1333-C7 (Perseus). With millimeter observations, we derived their column densities, the C and N isotopic fractions, the isomeric ratios, and the deuterium fractionation. The continuum data at 3 mm and 850 µm allowed us to compute the emissivity spectral index and look for grain growth as an evolutionary tracer.
Results. The H13CN/HN13C ratio is anticorrelated with the deuterium fraction of HCN, thus it can readily serve as a proxy for the temperature. The spectral index (β ∼ 1.34-2.09) shows a tentative anticorrelation with the H13CN/HN13C ratio, suggesting grain growth in the evolved, hotter, and less deuterated sources. Unlike TMC 1-C, the south-to-north gradient in dust temperature and spectral index observed in NGC 1333-C7 suggests feedback from the main NGC 1333 cloud.
Conclusions. With this up-to-date characterization of two star-forming regions, we found that the chemistry and the physical properties are tightly related. The dust temperature, deuterium fraction, and the spectral index are complementary evolutionary tracers. The large-scale environmental factors may dominate the chemistry and evolution in clustered star-forming regions.

Abstract Copyright: © The Authors 2023

Journal keyword(s): astrochemistry - astronomical databases: miscellaneous - molecular data - ISM: molecules - stars: formation - atomic data

Simbad objects: 17

goto Full paper

goto View the references in ADS

Number of rows : 17
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 LDN 1448 DNe 03 22.5 +30 35           ~ 546 0
2 LDN 1455 DNe 03 28 00.6480 +30 07 58.800           ~ 198 1
3 NGC 1333 OpC 03 29 09.2 +31 20 59           ~ 1575 1
4 JCMTPP J032917.2+312746 Y*O 03 29 17.17 +31 27 46.5           ~ 43 0
5 [KJD2006] SMM J032930+31251 cor 03 29 18.28 +31 25 06.3           ~ 21 0
6 JCMTSE J032918.7+312312 cor 03 29 19.04 +31 23 13.7           ~ 19 0
7 SSTc2d J032923.9+313320 cor 03 29 23.9 +31 33 20           ~ 14 1
8 [EYG2006] Bolo 58 cor 03 29 25.5 +31 28 18           ~ 68 0
9 Barnard 1 MoC 03 33 16.3 +31 07 51           ~ 350 0
10 NAME Perseus Cloud SFR 03 35.0 +31 13           ~ 1553 0
11 Barnard 213 DNe 04 20 51 +27 16.3           ~ 249 0
12 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
13 TMC-1 NH3 PoC 04 41 18.5 +25 48 14           ~ 20 0
14 TMC-1 CP Cld 04 41 34.97 +25 38 53.2           ~ 69 1
15 Barnard 220 DNe 04 41 38.8 +26 00 42           ~ 141 0
16 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0
17 LDN 1544 DNe 05 04 16.6 +25 10 48           ~ 965 0

To bookmark this query, right click on this link: simbad:objects in 2023A&A...670A.110N and select 'bookmark this link' or equivalent in the popup menu