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Your search keyword '"Etoka S"' showing total 62 results

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62 results on '"Etoka S"'

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1. Chemical tracers of a highly eccentric AGB–main-sequence star binary

2. ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA

3. Tracing Evolution in Massive Protostellar Objects (TEMPO) – I. Fragmentation and emission properties of massive star-forming clumps in a luminosity limited ALMA sample

4. ATOMIUM: Probing the inner wind of evolved O-rich stars with new, highly excited H2O and OH lines

5. The VLT/SPHERE view of the ATOMIUM cool evolved star sample

6. Flaring Masers and Pumping

12. ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars

14. The sharp ALMA view of infall and outflow in the massive protocluster G31.41+0.31

15. Evolutionary map of the Universe (EMU): 18-cm OH-maser discovery in ASKAP continuum images of the SCORPIO field

16. ATOMIUM: halide molecules around the S-type AGB star W Aquilae

17. Fragmentation in the massive G31.41+0.31 protocluster

19. (Sub)stellar companions shape the winds of evolved stars

24. Masers: Precision probes of molecular gas

26. Chasing discs around O-type (proto)stars

27. The feedback of an HC HII region on its parental molecular core

29. Accelerating infall and rotational spin-up in the hot molecular core G31.41+0.31

35. Simultaneous 183 GHz H2O maser and SiO observations towards evolved stars using APEX SEPIA Band 5

36. Magnetically aligned dust and SiO maser polarisation in the envelope of the red supergiant VY Canis Majoris

37. Chasing discs around O-type (proto)stars: Evidence from ALMA observations

41. ALMA sub-mm maser and dust distribution of VY Canis Majoris

42. Filamentary structure and Keplerian rotation in the high-mass star-forming region G35.03+0.35 imaged with ALMA

43. A necklace of dense cores in the high-mass star forming region G35.20−0.74 N: ALMA observations

45. e-MERLIN resolves Betelgeuse at λ 5 cm: hotspots at 5 R⋆

46. A candidate circumbinary Keplerian disk in G35.20–0.74 N: A study with ALMA

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