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20112026
most citedOGLE-2002-BLG-360: from a gravitational microlensing candidate to an overlooked red transient

101 citations · 826 across the 22 of their papers we have counts for

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astro-ph.SR2013★ 50 cited

IRC-10414: a bow-shock-producing red supergiant star

V. V. Gvaramadze, K. M. Menten, A. Y. Kniazev +5

Most runaway OB stars, like the majority of massive stars residing in their parent clusters, go through the red supergiant (RSG) phase during their lifetimes. Nonetheless, although…

astro-ph.SR2013★ 66 cited

An Interferometric Spectral-Line and Imaging Survey of VY Canis Majoris in the 345 GHz Band

T. Kaminski, C. A. Gottlieb, K. H. Young +2

A spectral line survey of the oxygen-rich red supergiant VY Canis Majoris was made between 279 and 355 GHz with the Submillimeter Array. Two hundred twenty three spectral features…

astro-ph.SR2013★ 93 cited

PO and PN in the wind of the oxygen-rich AGB star IK Tau

E. De Beck, T. Kamiński, N. A. Patel +4

Phosphorus-bearing compounds have only been studied in the circumstellar environments (CSEs) of the asymptotic giant branch (AGB) star IRC +10216 and the protoplanetary nebula CRL…

astro-ph.SR2013★ 15 cited

Optical spectropolarimetry of V4332 Sagittarii

T. Kamiński, R. Tylenda

The eruption of V4332 Sgr was observed in 1994. During the outburst, the object became extremely red, so it has been considered as to belong to red transients of the V838 Mon type.…

astro-ph.SR2013★ 101 cited

OGLE-2002-BLG-360: from a gravitational microlensing candidate to an overlooked red transient

R. Tylenda, T. Kaminski, A. Udalski +9

OGLE-2002-BLG-360 was discovered as a microlensing candidate by the OGLE-III project. The subsequent light curve however clearly showed that the brightening of the object could not…

astro-ph.SR2013★ 11 cited

Dust-forming molecules in VY Canis Majoris (and Betelgeuse)

T. Kaminski, C. A. Gottlieb, M. R. Schmidt +7

The formation of inorganic dust in circumstellar environments of evolved stars is poorly understood. Spectra of molecules thought to be most important for the nucleation, i.e. AlO,…