Published June 23, 2020 | Version v1
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Multifrequency study of HH 137 and HH 138: Discovering new knots and molecular outflows with Gemini and APEX

Creators

  • 1. Universidad Nacional de Córdoba, Observatorio Astronómico de Córdoba, Laprida 854, Córdoba X5000BGR, Argentina
  • 2. Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de la Plata, Paseo del Bosque s/n, 1900 La Plata, Argentina
  • 3. Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile

Description

We present reduced H2 and K near-infrared band images of HH 137, taken with the GSAOI+GeMS instrument of the Gemini South telescope. In addition, we provide submilimiter data in 12CO(3-2), 13CO(3-2), C18O(3-2), HCO+(3-2) and HCN(3-2) molecular lines of both HH 137 and HH 138, obtained with the SHeFI instrument of the Atacama Pathfinder EXperiment (APEX) telescope.

Notes

Accepted for publication in MNRAS

Files

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Additional details

Related works

Is derived from
Journal article: 10.1093/mnras/staa1863 (DOI)

References

  • Ferrero et al. 2020