activity
20182022
most citedHII regions and high-mass starless clump candidates II. Fragmentation and induced star formation at ~0.025 pc scale: An ALMA continuum study

37 citations · 113 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202224 cited

SFR estimations from z=0 to z=0.9 -- A comparison of SFR calibrators for star-forming galaxies

M. Figueira, A. Pollo, K. Małek +7

Using VIPERS, we estimated a set of SFR based on photometric and spectroscopic data. We used, as estimators, photometric bands from ultraviolet to mid-infrared, and spectral lines.…

astro-ph.GA202137 cited

HII regions and high-mass starless clump candidates II. Fragmentation and induced star formation at ~0.025 pc scale: An ALMA continuum study

S. Zhang, A. Zavagno, A. López-Sepulcre +7

The ionization feedback from HII regions modifies the properties of high-mass starless clumps (HMSCs, of several hundred to a few thousand solar masses with a size of ~0.1-1 pc), s…

astro-ph.GA202013 cited

APEX CO observations towards the photodissociation region of RCW120

Miguel Figueira, Annie Zavagno, Leonardo Bronfman +3

The edges of ionized (HII) regions are important sites for the formation of (high-mass) stars. Indeed, at least 30% of the galactic high mass star formation is observed there. The…

astro-ph.GA202033 cited

The role of Galactic HII regions in the formation of filaments. High-resolution submilimeter imaging of RCW 120 with ArTéMiS

A. Zavagno, Ph. André, F. Schuller +13

Massive stars and their associated ionized (HII) regions could play a key role in the formation and evolution of filaments that host star formation. However, the properties of fila…

astro-ph.GA2020

HII regions and high-mass starless clump candidates I: Catalogs and properties

S. Zhang, A. Zavagno, J. Yuan +6

The role of ionization feedback on high-mass (>8 Msun) star formation (HMSF) is still highly debated. Questions remain concerning the presence of nearby HII regions changes the pro…

astro-ph.GA20196 cited

Multiwavelength study of the G345.5+1.5 region

M. Figueira, C. López-Calderón, L. Bronfman +4

Star-forming regions are usually studied in the context of Galactic surveys, but dedicated observations are sometimes needed when the study reaches beyond the survey area. Here, we…