activity
20042022
most citedSpin down of the core rotation in red giants

463 citations · 1.6k across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.HE2022★ 22 cited

Timing properties of the X-ray accreting pulsar 1A 0535+262 studied with Insight-HXMT

P. J. Wang, L. D. Kong, S. Zhang +13

We report results on the timing analysis of the 2020 giant outburst of 1A 0535+262, using broadband data from Insight-HXMT. The analysis of the pulse profile evolution from the sub…

astro-ph.HE2021★ 14 cited

Simultaneous X-ray and radio observations of the transitional millisecond pulsar candidate CXOU J110926.4-650224. The discovery of a variable radio counterpart

F. Coti Zelati, B. Hugo, D. F. Torres +15

We present the results of simultaneous observations of the transitional millisecond pulsar (tMSP) candidate CXOU J110926.4-650224 with the XMM-Newton satellite and the MeerKAT tele…

astro-ph.GA2021★ 58 cited

An ALMA multi-line survey of the ISM in two quasar host-companion galaxy pairs at

A. Pensabene, R. Decarli, E. Bañados +15

We present a multi-line survey of the interstellar medium (ISM) in two quasar (QSO) host galaxies, PJ231-20 () and PJ308-21 (), and their two companion galaxi…

astro-ph.EP2021★ 13 cited

Rotational Mass Shedding from Asteroid (6478) Gault

J. X. Luu, D. C. Jewitt, M. Mutchler +4

The 4 km diameter main belt asteroid 6478 Gault has ejected dust intermittently since at least 2013. The character of the emission, including its episodic nature and the low…

astro-ph.HE2020★ 19 cited

Hints of gamma-ray orbital variability from gamma^2 Velorum

G. Martí-Devesa, O. Reimer, J. Li +1

Context. Colliding wind binaries are massive systems featuring strong, interacting stellar winds which may act as particle accelerators. Therefore, such binaries are good candidate…

astro-ph.GA2019★ 67 cited

A systematic TMRT observational study of Galactic C/C ratios from Formaldehyde

Y. T. Yan, J. S. Zhang, C. Henkel +10

We present observations of the C-band (4.8 GHz) and Ku-band (14.5 GHz) K-doublet lines of HCO and the C-band (4.6 GHz) line of H…