most citedInhomogeneous molecular ring around the B[e] supergiant LHA 120-S 73

27 citations · 37 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2023

Introducing the ASSESS project: Episodic Mass Loss in Evolved Massive Stars -- Key to Understanding the Explosive Early Universe

A. Z. Bonanos, G. Maravelias, M. Yang +6

Episodic mass loss is not understood theoretically, neither accounted for in state-of-the-art models of stellar evolution, which has far-reaching consequences for many areas of ast…

astro-ph.SR20162 cited

The yellow hypergiant - B[e] supergiant connection

Anna Aret, Michaela Kraus, Indrek Kolka +1

B[e] supergiants and yellow hypergiants share a number of common properties regarding their circumstellar environments. Using the forbidden [O I] and [Ca II] lines as disk tracers,…

astro-ph.SR20161 cited

A new outburst of the yellow hypergiant star Cas

Anna Aret, Michaela Kraus, Indrek Kolka +1

Spectroscopic monitoring of the yellow hypergiant Cas revealed a new outburst in 2013, which is obvious from the development of TiO bands in the spectra. Also many atmospheric…

astro-ph.SR20165 cited

Similarities in the structure of the circumstellar environments of B[e] supergiants and yellow hypergiants

Anna Aret, Indrek Kolka, Michaela Kraus +1

Yellow Hypergiants (YHGs) and B[e] supergiants (B[e]SGs), though in different phases in their evolution, display many features in common. This is partly due to the fact that both t…

astro-ph.SR2016

Clumpy molecular structures revolving the B[e] supergiant MWC 137

M. Kraus, L. S. Cidale, T. Liimets +10

The peculiar emission-line star MWC 137 with its extended optical nebula was recently classified as B[e] supergiant. To study the spatial distribution of its circumstellar molecula…

astro-ph.SR20162 cited

B[e] Supergiants' circumstellar environment: disks or rings?

G. Maravelias, M. Kraus, A. Aret +3

B[e] Supergiants are a phase in the evolution of some massive stars for which we have observational evidence but no predictions by any stellar evolution model. The mass-loss during…