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Ionize Hard: Interstellar PO + Detection

Rivilla, Víctor M. (author)
Centro de Astrobiologia (CAB)
García De La Concepción, Juan (author)
Centro de Astrobiologia (CAB)
Jimenez-Serra, I. (author)
Centro de Astrobiologia (CAB)
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Martin-Pintado, J. (author)
Centro de Astrobiologia (CAB)
Colzi, L. (author)
Centro de Astrobiologia (CAB)
Tercero, B. (author)
Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)
Megías, Andrés (author)
Centro de Astrobiologia (CAB)
López-Gallifa, Álvaro (author)
Centro de Astrobiologia (CAB)
Martínez-Henares, Antonio (author)
Centro de Astrobiologia (CAB)
Massalkhi, Sara (author)
Centro de Astrobiologia (CAB)
Martin, S. (author)
European Southern Observatory Santiago,Atacama Large Millimeter-submillimeter Array (ALMA)
Zeng, Shaoshan (author)
RIKEN
Vicente, P. de (author)
Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)
Rico-Villas, Fernando (author)
Centro de Astrobiologia (CAB)
Requena-Torres, M. A. (author)
University of Maryland,Towson University
Cosentino, Giuliana, 1990 (author)
Chalmers tekniska högskola,Chalmers University of Technology
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 (creator_code:org_t)
2022-04-26
2022
English.
In: Frontiers in Astronomy and Space Sciences. - : Frontiers Media SA. - 2296-987X. ; 9
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We report the first detection of the phosphorus monoxide ion (PO+) in the interstellar medium. Our unbiased and very sensitive spectral survey toward the G+0.693–0.027 molecular cloud covers four different rotational transitions of this molecule, two of which (J = 1–0 and J = 2–1) appear free of contamination from other species. The fit performed, assuming local thermodynamic equilibrium conditions, yields a column density of N=(6.0 ± 0.7) × 1011 cm−2. The resulting molecular abundance with respect to molecular hydrogen is 4.5 × 10–12. The column density of PO+ normalized by the cosmic abundance of P is larger than those of NO+ and SO+, normalized by N and S, by factors of 3.6 and 2.3, respectively. The N(PO+)/N(PO) ratio is 0.12 ± 0.03, more than one order of magnitude higher than that of N(SO+)/N(SO) and N(NO+)/N(NO). These results indicate that P is more efficiently ionized than N and S in the ISM. We have performed new chemical models that confirm that the PO+ abundance is strongly enhanced in shocked regions with high values of cosmic-ray ionization rates (10–15 − 10–14 s−1), as occurring in the G+0.693–0.027 molecular cloud. The shocks sputter the interstellar icy grain mantles, releasing into the gas phase most of their P content, mainly in the form of PH3, which is converted into atomic P, and then ionized efficiently by cosmic rays, forming P+. Further reactions with O2 and OH produces PO+. The cosmic-ray ionization of PO might also contribute significantly, which would explain the high N(PO+)/N(PO) ratio observed. The relatively high gas-phase abundance of PO+ with respect to other P-bearing species stresses the relevance of this species in the interstellar chemistry of P.

Subject headings

NATURVETENSKAP  -- Kemi -- Fysikalisk kemi (hsv//swe)
NATURAL SCIENCES  -- Chemical Sciences -- Physical Chemistry (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)
NATURVETENSKAP  -- Kemi -- Annan kemi (hsv//swe)
NATURAL SCIENCES  -- Chemical Sciences -- Other Chemistry Topics (hsv//eng)

Keyword

phosphorus
interstellar: clouds
astrochemistry
interstellar: ions
interstellar: abundances

Publication and Content Type

art (subject category)
ref (subject category)

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