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Sökning: WFRF:(Nakatani K) > (2020-2021) > Chemical Complexity...

Chemical Complexity of Phosphorous-bearing Species in Various Regions of the Interstellar Medium

Sil, Milan (författare)
Indian Centre for Space Physics
Srivastav, Satyam (författare)
Banaras Hindu University
Bhat, Bratati (författare)
Indian Centre for Space Physics
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Mondal, Suman Kumar (författare)
Indian Centre for Space Physics
Gorai, Prasanta, 1991 (författare)
Chalmers tekniska högskola,Chalmers University of Technology,Indian Centre for Space Physics
Ghosh, Rana (författare)
Indian Centre for Space Physics
Shimonishi, Takashi (författare)
Niigata University
Chakrabarti, Sandip K. (författare)
Indian Centre for Space Physics
Sivaraman, Bhalamurugan (författare)
Physical Research Laboratory
Pathak, Amit (författare)
Banaras Hindu University
Nakatani, Naoki (författare)
Tokyo Metropolitan University,Hokkaido University
Furuya, Kenji (författare)
National Astronomical Observatory of Japan,University of Tsukuba
Das, Ankan (författare)
Indian Centre for Space Physics
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 (creator_code:org_t)
2021-08-25
2021
Engelska.
Ingår i: Astronomical Journal. - : American Astronomical Society. - 1538-3881 .- 0004-6256. ; 162:3
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
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  • Phosphorus-related species are not known to be as omnipresent in space as hydrogen, carbon, nitrogen, oxygen, and sulfur-bearing species. Astronomers spotted very few P-bearing molecules in the interstellar medium and circumstellar envelopes. Limited discovery of the P-bearing species imposes severe constraints in modeling the P-chemistry. In this paper, we carry out extensive chemical models to follow the fate of P-bearing species in diffuse clouds, photon-dominated or photodissociation regions (PDRs), and hot cores/corinos. We notice a curious correlation between the abundances of PO and PN and atomic nitrogen. Since N atoms are more abundant in diffuse clouds and PDRs than in the hot core/corino region, PO/PN reflects <1 in diffuse clouds, MUCH LESS-THAN1 in PDRs, and >1 in the late warm-up evolutionary stage of the hot core/corino regions. During the end of the post-warm-up stage, we obtain PO/PN > 1 for hot core and <1 for its low-mass analog. We employ a radiative transfer model to investigate the transitions of some of the P-bearing species in diffuse cloud and hot core regions and estimate the line profiles. Our study estimates the required integration time to observe these transitions with ground-based and space-based telescopes. We also carry out quantum chemical computation of the infrared features of PH3, along with various impurities. We notice that SO2 overlaps with the PH3 bending-scissoring modes around similar to 1000-1100 cm(-1). We also find that the presence of CO2 can strongly influence the intensity of the stretching modes around similar to 2400 cm(-1) of PH3.

Ämnesord

NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Meteorologi och atmosfärforskning (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Meteorology and Atmospheric Sciences (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Geologi (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Geology (hsv//eng)

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