activity
20142026
most citedDirect measurements of carbon and sulfur isotope ratios in the Milky Way

69 citations · 695 across the 51 of their papers we have counts for

collaborators
Showing 2025Show all

7 papers · 1 filter

astro-ph.GA2025

A global view on star formation: The GLOSTAR Galactic plane survey XII. Effelsberg's continuum view and data release

Y. Gong, W. Reich, M. R. Rugel +24

Extended radio continuum emission and its linear polarization play a key role in probing large-scale structures of synchrotron and free-free emission in the Milky Way. Despite the…

astro-ph.GA2025

A targeted radio survey of infrared-selected bow shock candidates

M. Moutzouri, J. Mackey, N. Castro +8

Bow shocks around massive stars have primarily been detected in IR emission, but radio detections are becoming more frequent with the commissioning of sensitive and large field-of-…

astro-ph.CO2025★ 1 cited

Probing cosmic velocities with the pairwise kinematic Sunyaev-Zel'dovich signal in DESI Bright Galaxy Sample DR1 and ACT DR6

B. Hadzhiyska, Y. Gong, Y. Hsu +55

We present a measurement of the pairwise kinematic Sunyaev-Zel'dovich (kSZ) signal using the Dark Energy Spectroscopic Instrument (DESI) Bright Galaxy Sample (BGS) Data Release 1 (…

astro-ph.GA2025★ 1 cited

Ammonia in the hot core W51-IRS2: Maser line profiles, variability, and saturation

E. Alkhuja, C. Henkel, Y. T. Yan +6

W51-IRS2 is known to be one of the most prolific sources of interstellar ammonia (NH) maser lines. So far, however, many of these inversion lines have rarely been studied. Here…

astro-ph.SR2025

New submillimetre HCN lasers in carbon-rich evolved stars

W. Yang, K. T. Wong, H. Wiesemeyer +6

Strong laser emission from hydrogen cyanide (HCN) at 805 and 891 GHz has been discovered towards carbon-rich (C-rich) AGB stars, originating from the Coriolis-coupled system betwee…

astro-ph.GA2025★ 4 cited

Shock-induced HCNH+ abundance enhancement in the heart of the starburst galaxy NGC 253 unveiled by ALCHEMI

Y. Gong, C. Henkel, C. T. Bop +15

Understanding the chemistry of molecular clouds is pivotal to elucidate star formation and galaxy evolution. As one of the important molecular ions, HCNH+ plays an important role i…

astro-ph.SR2025★ 3 cited

Molecular inventory of a young eruptive star's environment -- Case study of the classical FU Orionis star V1057 Cyg

Zs. M. Szabó, A. Belloche, K. M. Menten +6

Studying accretion-driven episodic outbursts in YSOs is key to understanding the later stages of star and planet formation. FU Orionis-type objects form a YSO subclass, distinguish…