Millimeter and submillimeter spectroscopy of the deuterated molecular ion SD+
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arXiv
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| Auteurs principaux: | , , , |
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| Format: | Preprint |
| Publié: |
2024
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| _version_ | 1866911809189969920 |
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| author | Araki, Mitsunori Lattanzi, Valerio Endres, Christian P. Caselli, Paula |
| author_facet | Araki, Mitsunori Lattanzi, Valerio Endres, Christian P. Caselli, Paula |
| contents | Seven rotational and fine-structure transitions of the deuterated molecular ion SD+ in the X 3S- ground electronic state have been measured in the 271-863 GHz region in the laboratory. This ion has been produced by DC-glow discharge using a mixture of D2S and argon in a free space cell in a temperature range of -140 to -160C. The rotational, centrifugal distortion, spin-spin interaction, and hyperfine constants have been determined; the standard deviation of the residuals in the fitting is 109 kHz. The set of obtained spectroscopic parameters provides a list of accurate sub-millimeter rest frequencies of SD+ for astronomical detection. We have investigated lines of SD+ toward the quasar PKS 1830-211 using the ALMA archive, as the z = 0.89 molecular absorber exists in front of this quasar. A data set covering the 297 GHz region includes the N_J = 2_3-1_2 transition at 561 GHz due to redshift, providing an upper limit of the column density Ntot = 3 x 10^12 cm-2 for SD+. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2403_15035 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Millimeter and submillimeter spectroscopy of the deuterated molecular ion SD+ Araki, Mitsunori Lattanzi, Valerio Endres, Christian P. Caselli, Paula Astrophysics of Galaxies Solar and Stellar Astrophysics Seven rotational and fine-structure transitions of the deuterated molecular ion SD+ in the X 3S- ground electronic state have been measured in the 271-863 GHz region in the laboratory. This ion has been produced by DC-glow discharge using a mixture of D2S and argon in a free space cell in a temperature range of -140 to -160C. The rotational, centrifugal distortion, spin-spin interaction, and hyperfine constants have been determined; the standard deviation of the residuals in the fitting is 109 kHz. The set of obtained spectroscopic parameters provides a list of accurate sub-millimeter rest frequencies of SD+ for astronomical detection. We have investigated lines of SD+ toward the quasar PKS 1830-211 using the ALMA archive, as the z = 0.89 molecular absorber exists in front of this quasar. A data set covering the 297 GHz region includes the N_J = 2_3-1_2 transition at 561 GHz due to redshift, providing an upper limit of the column density Ntot = 3 x 10^12 cm-2 for SD+. |
| title | Millimeter and submillimeter spectroscopy of the deuterated molecular ion SD+ |
| topic | Astrophysics of Galaxies Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2403.15035 |