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Telluric absorption lines in the ALMA spectra of eta Car

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Autor(es):
Abraham, Zulema ; Beaklini, Pedro P. B. ; Cox, Pierre ; Falceta-Goncalves, Diego ; Nyman, Lars-Ake
Número total de Autores: 5
Tipo de documento: Artigo Científico
Fonte: Monthly Notices of the Royal Astronomical Society; v. 517, n. 1, p. 12-pg., 2022-10-04.
Resumo

The massive binary system formed by eta Car and an unknown companion is a strong source at millimetre and submillimetre wavelengths. Close to the stars, continuum bremsstrahlung and radio recombination lines originate in the massive ionized wind of eta Car and in several compact sources of high density plasma. Molecular lines are also detected at these wavelengths, some of them are seen in absorption towards the continuum emission region, many of them revealed by ALMA observations. However, because the ALMA atmospheric calibration is performed in a low spectral resolution mode, telluric lines can still be present in some high-resolution spectra of scientific products, which could lead to a false identification of molecules. In this work, we explore three different sets of ALMA archive data of eta Car, including high resolution (0.065 arcsec x 0.043 arcsec) observations recently published by our group, to verify which of these absorption lines are real and discuss their origin. We conclude that some of them truly originate in clouds close to the binary system, while others are artefacts of a faulty elimination of telluric lines during ALMA calibration procedure. We found that these absorption lines are not present in the phase calibrators because they are much weaker than eta Car, where the absorption line appears because the high intensity continuum enhances the small individual systematic calibration errors. (AU)

Processo FAPESP: 14/07460-0 - Alvos para o LLAMA: estudo da variabilidade de rádio fontes em 43 GHz (banda 1) e busca por correlação com imagens interferométricas
Beneficiário:Pedro Paulo Bonetti Beaklini
Modalidade de apoio: Bolsas no Brasil - Pós-Doutorado
Processo FAPESP: 11/51676-9 - LLAMA: um radiotelescópio para ondas mm/sub-mm nos Andes, em colaboração com a Argentina
Beneficiário:Jacques Raymond Daniel Lépine
Modalidade de apoio: Auxílio à Pesquisa - Temático