activity
20012017
most citedA Very Large Array 3.6cm continuum survey of Galactic Wolf-Rayet stars

67 citations · 327 across the 17 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2017★ 20 cited

Resolving the circumstellar environment of the Galactic B[e] supergiant star MWC 137 from large to small scales

Michaela Kraus, Tiina Liimets, Cristina E. Cappa +10

The Galactic object MWC 137 was suggested to belong to the group of B[e] supergiants. However, with its large-scale optical bipolar ring nebula and the high velocity jet and knots,…

astro-ph.GA2017

Molecular and Atomic Clouds toward the Wolf-Rayet Nebula NGC 2359: Possible Evidence for Isolated High-Mass Star Formation Triggered by a Cloud-Cloud Collision

Hidetoshi Sano, Katsuhiro Hayashi, Rei Enokiya +17

NGC 2359 is an HII region located in the outer Galaxy that contains the isolated Wolf-Rayet (WR) star HD 56925. We present millimeter/submillimeter observations of CO( =…

astro-ph.GA2017★ 16 cited

Triggered massive star formation associated with the bubble HII region Sh2-39 (N5)

N. U. Duronea, C. E. Cappa, L. Bronfman +2

Aiming at studying the physical properties of Galactic IR bubbles and to explore their impact in triggering massive star formation, we perform a multiwavelength analysis of the bub…

astro-ph.GA2016

A submillimeter study of the IR dust bubble S 21 and its environs

C. E. Cappa, N. U. Duronea, J. Vasquez +4

Based on the molecular emission in the CO(2-1) and CO(2-1) lines, and the continuum emission in the MIR and FIR towards the S21 IR dust bubble, we analyze the physica…

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.GA2015★ 7 cited

Molecular gas and star formation towards the IR dust bubble S24 and its environs

C. E. Cappa, N. U. Duronea, V. Firpo +4

We present a multi-wavelength analysis of the infrared dust bubble S24, and its environs, with the aim of investigating the characteristics of the molecular gas and the interstella…