activity
20162026
most citedEpisodic accretion: the interplay of infall and disc instabilities

106 citations · 399 across the 21 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2026

Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds

Andrea Bracco, Tyler L. Bourke, Stefano Bovino +8

Magnetic fields play a central role in the star-formation process, from diffuse gas to the dense, starless, molecular cloud cores that represent the first gravitationally bound str…

astro-ph.GA2024★ 14 cited

PRODIGE -- envelope to disk with NOEMA. IV. An infalling gas bridge surrounding two Class 0/I systems in L1448N

C. Gieser, J. E. Pineda, D. M. Segura-Cox +13

Context. The formation of stars has been subject to extensive studies in the past decades from molecular cloud to protoplanetary disk scales. It is still not fully understood how t…

astro-ph.GA2024★ 5 cited

Probing the Physics of Star-Formation (ProPStar) III. No evidence for dissipation of turbulence down to 20 mpc (4 000 au) scale

Jaime E. Pineda, Juan D. Soler, Stella Offner +14

Context. Turbulence is a key component of molecular cloud structure. It is usually described by a cascade of energy down to the dissipation scale. The power spectrum for subsonic i…

astro-ph.GA2024★ 25 cited

Probing the Physics of Star-Formation (ProPStar): II. The first systematic search for streamers toward protostars

María Teresa Valdivia-Mena, Jaime E. Pineda, Paola Caselli +9

The detection of narrow channels of accretion toward protostellar disks, known as streamers, have increased in number in the last few years. However, it is unclear if streamers are…

astro-ph.GA2024★ 31 cited

Probing the physics of star formation (ProPStar): I. First resolved maps of the electron fraction and cosmic-ray ionization rate in NGC 1333

Jaime E. Pineda, Olli Sipilä, Dominique M. Segura-Cox +11

Electron fraction and cosmic-ray ionization rates (CRIR) in star-forming regions are important quantities in astrochemical modeling and are critical to the degree of coupling betwe…