Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. First Detection of Silicon-bearing Molecules in η Car
 

First Detection of Silicon-bearing Molecules in η Car

Journal
THE ASTROPHYSICAL JOURNAL LETTERS  
Date Issued
2022
Author(s)
Bordiu, C.
•
Rizzo, J. R.
•
BUFANO, FILOMENA  
•
Quintana-Lacaci, G.
•
BUEMI, CARLA SIMONA  
•
LETO, PAOLO  
•
CAVALLARO, Francesco  
•
Cerrigone, L.
•
INGALLINERA, Adriano  
•
LORU, Sara  
•
RIGGI, Simone  
•
TRIGILIO, CORRADO  
•
UMANA, Grazia Maria Gloria  
•
SCIACCA, Eva  
DOI
10.3847/2041-8213/ac9b10
Abstract
We present ALMA band 6 observations of the luminous blue variable η Car obtained within the ALMAGAL program. We report SiO J = 5 → 4, SiS J = 12 → 11, and SiN N = 5 → 4 emission in the equatorial region of the Homunculus nebula, constituting the first detection of silicon- and sulfur-bearing molecules in the outskirts of a highly evolved, early-type massive star. The SiO, SiS, and SiN trace a clumpy equatorial ring that surrounds the central binary at a projected distance of ∼2″, delineating the inner rims of the butterfly-shaped dusty region. The formation of silicon-bearing compounds is presumably related to the continuous recycling of dust due to the variable wind regime of η Car, which destroys grains and releases silicon back to the gas phase. We discuss possible formation routes for the observed species, contextualizing them within the current molecular inventory of η Car. We find that the SiO and SiS fractional abundances in localized clumps of the ring, 6.7 × 10−9 and 1.2 × 10−8, respectively, are exceptionally lower than those measured in C- and O-rich AGB stars and cool supergiants, while the higher SiN abundance, 3.6 × 10−8, evidences the nitrogen-rich chemistry of the ejecta. These abundances must be regarded as strict upper limits, since the distribution of H2 in the Homunculus is unknown. In any case, these findings shed new light on the peculiar molecular ecosystem of η Car and establish its surroundings as a new laboratory to investigate the life cycle of silicate dust in extreme astrophysical conditions.
Volume
939
Issue
2
Start page
L30
Uri
http://hdl.handle.net/20.500.12386/32888
Url
https://iopscience.iop.org/article/10.3847/2041-8213/ac9b10
Issn Identifier
2041-8205
Ads BibCode
2022ApJ...939L..30B
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

Bordiu_2022_ApJL_939_L30.pdf

Description
Pdf editoriale
Size

1009.06 KB

Format

Adobe PDF

Checksum (MD5)

682becaad10530b3c3a93218537dc195

Loading...
Thumbnail Image
Name

2210.09774.pdf

Description
arXiv
Size

918.46 KB

Format

Adobe PDF

Checksum (MD5)

695c819c145deb856786bb5b856ae2b1

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback