activity
20042023
most citedDetection of C60 in the proto-planetary nebula IRAS 01005+7910

131 citations · 1.7k across the 65 of their papers we have counts for

collaborators

65 papers

astro-ph.GA2023★ 115 cited

PDRs4All IV. An embarrassment of riches: Aromatic infrared bands in the Orion Bar

Ryan Chown, Ameek Sidhu, Els Peeters +136

(Abridged) Mid-infrared observations of photodissociation regions (PDRs) are dominated by strong emission features called aromatic infrared bands (AIBs). The most prominent AIBs ar…

astro-ph.SR2023★ 4 cited

A 3 mm Molecular Line Survey toward The C-star Envelope CIT 6

Kui-Lu Yang, Yong Zhang, Jian-Jie Qiu +2

We present an unbiased molecular line survey toward the carbon-rich circumstellar envelope CIT 6 carried out between 90 and 116 GHz with the Arizona Radio Observatory 12 m telescop…

astro-ph.SR2023

Photochemical origin of SiC in the circumstellar envelope of carbon-rich AGB stars revealed by ALMA

Yanan Feng, Xiaohu Li, Tom J. Millar +16

Whether SiC is a parent species, that is formed in the photosphere or as a by-product of high-temperature dust formation, or a daughter species, formed in a chemistry driven by…

astro-ph.GA2023★ 43 cited

Direct observational evidence of the multi-scale, dynamical mass accretion toward a high-mass star forming hub-filament system

Dongting Yang, Hong-Li Liu, Anandmayee Tej +28

There is growing evidence that high-mass star formation and hub-filament systems (HFS) are intricately linked. The gas kinematics along the filaments and the forming high-mass star…

astro-ph.SR2023★ 2 cited

FAST search for circumstellar atomic hydrogen. II. Is BD+303639 an interacting planetary nebula?

Xu-Jia Ouyang, Yong Zhang, Albert Zijlstra +3

The young, compact, very high surface brightness but low excitation planetary nebula (PN) BD+303639 is one of the very few PNe that have been reported to exhibit the 21cm HI emissi…

astro-ph.GA2023★ 55 cited

Evidence of high-mass star formation through multi-scale mass accretion in hub-filament-system clouds

Hong-Li Liu, Anandmayee Tej, Tie Liu +30

We present a statistical study of a sample of 17 hub-filament-system (HFS) clouds of high-mass star formation using high-angular resolution (1-2 arcsecond) ALMA 1.3mm and 3mm…