Figure 1 from Interferometric Imaging of Titan’s HC3N, H13CCCN, and HCCC15N

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Interferometric Imaging of Titan’s HC₃N, H¹³CCCN, and HCCC¹⁵N

Authors: M. A. Cordiner, C. A. Nixon, S. B. Charnley, N. A. Teanby, E. M. Molter, Z. Kisiel, and V. Vuitton

2018 The Astrophysical Journal Letters 859 L15.

Provider: AAS Journals

Caption: Figure 1.

ALMA spectra of HC₃N extracted from a beam centered 200 km above the south polar limb, including the (J = 39 − 38, v = 0) rotational transition of the vibrational ground state, the (J = 39 − 38, v₇ = 1f) transition of the vibrationally excited state, and the ground-state rotational transitions of the detected ¹³C and ¹⁵N isotopologues (see Table 1).

Other Images in This Article

Copyright and Terms & Conditions