output
19922026
most citedSkyrmion Lattice in a Chiral Magnet

4.8k citations

Showing 2018 · astro-ph.SRShow all

17 papers · 2 filters

astro-ph.SR2018★ 14 cited

Evolution of Hubble wedges in episodic protostellar outflows

P. F. Rohde, S. Walch, D. Seifried +2

Young low-mass protostars undergo short phases of high accretion and outburst activity leading to lumpy outflows. Recent observations have shown that the position-velocity and mass…

astro-ph.SR2018★ 12 cited

Deuterated methyl mercaptan (CHSD): Laboratory rotational spectroscopy and search toward IRAS 16293-2422 B

Olena Zakharenko, Frank Lewen, Vadim V. Ilyushin +4

Methyl mercaptan (also known as methanethiol), CH3SH, has been found in the warm and dense parts of high -- as well as low -- mass star-forming regions. The aim of the present stud…

astro-ph.SR2018★ 34 cited

Laboratory spectroscopic study of isotopic thioformaldehyde, HCS, and determination of its equilibrium structure

H. S. P. Müller, A. Maeda, S. Thorwirth +6

Thioformaldehyde is an abundant molecule in various regions of the interstellar medium. However, available laboratory data limit the accuracies of calculated transition frequencies…

astro-ph.SR2018★ 51 cited

The ALMA-PILS survey: The first detection of doubly-deuterated methyl formate (CHD2OCHO) in the ISM

S. Manigand, H. Calcutt, J. K. Jørgensen +9

Studies of deuterated isotopologues of complex organic molecules can provide important constraints on their origin in regions of star formation. In particular, the abundances of de…

astro-ph.SR2018★ 21 cited

NU Ori: a hierarchical triple system with a strongly magnetic B-type star

M. Shultz, J. -B. Le Bouquin, Th. Rivinius +13

NU Ori is a massive spectroscopic and visual binary in the Orion Nebula Cluster, with 4 components: Aa, Ab, B, and C. The B0.5 primary (Aa) is one of the most massive B-type stars…

astro-ph.SR2018★ 64 cited

Chasing discs around O-type (proto)stars - ALMA evidence for an SiO disc and disc wind from G17.64+0.16

L. T. Maud, R. Cesaroni, M. S. N. Kumar +28

We present high angular resolution 0.2 arcsec continuum and molecular emission line Atacama Large Millimeter/sub-millimeter Array (ALMA) observations of G17.64+0.16 in Band 6 (220G…