Alma observations of fragmentation, substructure, and protostars in high-mass starless clump candidates

Brian E. Svoboda, Yancy L. Shirley, Alessio Traficante, Cara Battersby, Gary A. Fuller, Qizhou Zhang, Henrik Beuther, Nicolas Peretto, Crystal Brogan, Todd Hunter

Research output: Contribution to journalArticlepeer-review

37 Scopus citations


The initial physical conditions of high-mass stars and protoclusters remain poorly characterized. To this end, we present the first targeted ALMA Band 6 1.3 mm continuum and spectral line survey toward high-mass starless clump candidates, selecting a sample of 12 of the most massive candidates (4 ×102 M⊙Mc1 ≲4 × 103 M⊙) within d⊙ < 5 kpc. The joint 12 + 7 m array maps have a high spatial resolution of ≲3000 au (0.015 pc, θsyn≈0 8) and have high point-source mass-completeness down to M ≈ 0.3 M⊙ at 6σrms (or 1srms column density sensitivity of N=1.1 × 1022 cm-2). We discover previously undetected signposts of low-luminosity star formation from CO J = 2 → 1 and SiO J = 5 → 4 bipolar outflows and other signatures toward 11 out of 12 clumps, showing that current MIR/FIR Galactic plane surveys are incomplete to low- and intermediate-mass protostars (Lbol ≲ 50 L⊙), and emphasizing the necessity of high-resolution follow-up. We compare a subset of the observed cores with a suite of radiative transfer models of starless cores. We find a high-mass starless core candidate with a model-derived mass consistent with 2952 15 M⊙ when integrated over size scales of R < 2 × 104 au. Unresolved cores are poorly fit by radiative transfer models of externally heated Plummer density profiles, supporting the interpretation that they are protostellar even without detection of outflows. A high degree of fragmentation with rich substructure is observed toward 10 out of 12 clumps. We extract sources from the maps using a dendrogram to study the characteristic fragmentation length scale. Nearest neighbor separations, when corrected for projection with Monte Carlo random sampling, are consistent with being equal to the clump average thermal Jeans length (λj,th; i.e., separations equal to 0.4-1.6 × λj,th). In the context of previous observations that, on larger scales, see separations consistent with the turbulent Jeans length or the cylindrical thermal Jeans scale (≈3-4 × λj,th), our findings support a hierarchical fragmentation process, where the highest-density regions are not strongly supported against thermal gravitational fragmentation by turbulence or magnetic fields.

Original languageEnglish (US)
Article number36
JournalAstrophysical Journal
Issue number1
StatePublished - Nov 20 2019

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


Dive into the research topics of 'Alma observations of fragmentation, substructure, and protostars in high-mass starless clump candidates'. Together they form a unique fingerprint.

Cite this