Discovery of a new bona fide luminous blue variable in Norma

Abstract

We report the results of optical spectroscopy of the candidate evolved massive star MN44 revealed via detection of a circular shell with the Spitzer Space Telescope. First spectra taken in 2009 May--June showed the Balmer lines in emission as well as numerous emission lines of iron, which is typical of luminous blue variables (LBVs) near the visual maximum. New observations carried out in 2015 May--September detected significant changes in the spectrum, indicating that the star became hotter. We found that these changes are accompanied by significant brightness variability of MN44. In particular, the I_c-band brightness decreased by \approx 1.6 mag during the last six years and after reaching its minimum in 2015 June has started to increase. Using archival data, we also found that the I_c-band brightness increased by \approx 3 mag in \approx 30 yr preceding our observations. MN44 therefore represents the seventeenth known example of the Galactic bona fide LBVs. We detected a nitrogen-rich knot to the northwest of the star, which might represent an interstellar cloudlet interacting with the circumstellar shell. We discuss a possible association between MN44 and the INTEGRAL transient source of hard X-ray emission IGR J16327-4940, implying that MN44 might be either a colliding-wind binary or a high-mass X-ray binary.

13 pages, 7 figures, accepted for publication in MNRAS

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Cited by in corpus (8)

• MN48: a new Galactic bona fide luminous blue variable revealed by Spitzer and SALT
• On the Gaia DR2 distances for Galactic Luminous Blue Variables
• The 2018 Census of Luminous Blue Variables
• New luminous blue variable candidates in the NGC 247 galaxy
• A deep near-infrared spectroscopic survey of the Scutum-Crux arm for Wolf-Rayet stars
• MN44: a luminous blue variable running away from Westerlund 1
• Circumstellar structures around high-mass X-ray binaries
• Modeling the Remnants of Core-collapse Supernovae from Luminous Blue Variable stars