Observations of interstellar HOCO+: abundance enhancements toward the galactic center

Astrophys J. 1988 Nov 1;334(1):175-81. doi: 10.1086/166827.

Abstract

A survey of the 4(04)-3(03) and 1(01)-0(00) transitions of HOCO+ has been made toward several molecular clouds. The HOCO+ molecule was not observed in any sources except Sgr B2 and Sgr A. The 5(05)-4(04) and 4(14)-3(13) transitions were also detected toward Sgr B2. The results indicate that gas phase CO2 is not a major carbon reservoir in typical molecular clouds. In Sgr B2, the HOCO+ antenna temperature exhibits a peak approximately 2' north of the Sgr B2 central position (Sgr B2[M]) and the 4(04)-3(03) line emission is extended over a approximately 10' x 10' region. The column density of HOCO+ at the northern peak in Sgr B2 is approximately 3 x 10(14) cm-2, and the fractional abundance relative to H2 > or = 3 x 10(-10), which is about 2 orders of magnitude greater than recent predictions of quiescent cloud ion-molecule chemistry.

Publication types

  • Research Support, U.S. Gov't, Non-P.H.S.
  • Research Support, U.S. Gov't, P.H.S.

MeSH terms

  • Astronomical Phenomena
  • Astronomy
  • Carbon Dioxide / analysis
  • Carbon Dioxide / chemistry*
  • Chemical Phenomena
  • Chemistry
  • Extraterrestrial Environment*
  • Ions
  • Spectrum Analysis

Substances

  • Ions
  • Carbon Dioxide