activity
20032025
most citedA map of the day-night contrast of the extrasolar planet HD 189733b

816 citations · 3.4k across the 38 of their papers we have counts for

collaborators

35 papers

astro-ph.GA2025★ 2 cited

Bowshocks driven by the pole-on molecular jet of outbursting protostar SVS 13

G. Blázquez-Calero, G. Anglada, S. Cabrit +13

Outflows play a key role in the star and planet formation processes. Some outflows show discrete clumps of cold molecular gas moving at extremely high velocities (EHVs) of 10…

astro-ph.SR2025

JWST observations of segregated CO and CO ices in protostellar envelopes

N. G. C. Brunken, A. C. A. Boogert, E. F. van Dishoeck +13

The evolution of interstellar ices can be studied with thermal tracers such as the vibrational modes of CO ice that show great diversity depending on their local chemical and t…

astro-ph.GA2024★ 23 cited

On the magnetic field properties of protostellar envelopes in Orion

Bo Huang, Josep M. Girart, Ian W. Stephens +23

We present 870 um polarimetric observations toward 61 protostars in the Orion molecular clouds, with ~400 au (1") resolution using the Atacama Large Millimeter/submillimeter Array.…

astro-ph.GA2024★ 43 cited

Hunt for complex cyanides in protostellar ices with JWST: Tentative detection of CHCN and CHCN

P. Nazari, W. R. M. Rocha, A. E. Rubinstein +20

Nitrogen-bearing complex organic molecules have been commonly detected in the gas phase but not yet in interstellar ices. This has led to the long-standing question of whether thes…

astro-ph.GA2022★ 22 cited

Low Mass Stars as Tracers of Star and Cluster Formation

S. T. Megeath, R. A. Gutermuth, M. A. Kounkel

We review the use of young low mass stars and protostars, or young stellar objects (YSOs), as tracers of star formation. Observations of molecular clouds at visible, infrared, radi…

astro-ph.SR2022★ 42 cited

The Rate, Amplitude and Duration of Outbursts from Class 0 Protostars in Orion

W. Zakri, S. T. Megeath, W. J. Fischer +18

At least half of a protostar's mass is accreted in the Class 0 phase, when the central protostar is deeply embedded in a dense, infalling envelope. We present the first systematic…