Density substructure is expected in evolved starless cores: a single peak to form a protostar, or multiple peaks from fragmentation. Searches for this substructure have had mixed success. In an ALMA survey of Ophiuchus, we find two starless cores with signs of substructure, consistent with simulation predictions. A similar survey in Chameleon (Dunham et al. 2016) had no detections, despite expecting at least two. Our results suggest that Chamleon may lack a more evolved starless cores. Future ALMA observations will better trace the influence of environment on core substructure formation
We present an unbiased census of starless cores in Perseus, Serpens, and Ophiuchus, assembled by com...
Although the standard model of star formation has served us well for over 20 years, its details are ...
In this paper, we present the results of a high resolution (5'') Combined Array for Research in Mill...
Density substructure is expected in evolved starless cores: a single peak to form a protostar, or mu...
Compact substructure is expected to arise in a starless core as mass becomes concentrated in the cen...
We present an Atacama Large Millimeter/submillimeter Array (ALMA) 106 GHz (Band 3) continuum survey ...
We present an Atacama Large Millimeter/submillimeter Array (ALMA) 106 GHz (Band 3) continuum survey ...
We present SMA and CARMA continuum and spectral line observations of five dense cores located in the...
The initial physical conditions of high-mass stars and protoclusters remain poorly characterized. To...
While clearly a vital step in the process of star formation, the transition from prestellar core to ...
Interpreting the nature of starless cores has been a prominent goal in star formation for many years...
The nearby Chamaeleon molecular cloud complex is a good laboratory to study the process of low-mass ...
Context. Chamaeleon I is the most active region in terms of star formation in the Chamaeleon molecul...
Chamaeleon I is the most active region in terms of star formation in the Chamaeleon molecular cloud ...
We present an unbiased census of starless cores in Perseus, Serpens, and Ophiuchus, assembled by com...
Although the standard model of star formation has served us well for over 20 years, its details are ...
In this paper, we present the results of a high resolution (5'') Combined Array for Research in Mill...
Density substructure is expected in evolved starless cores: a single peak to form a protostar, or mu...
Compact substructure is expected to arise in a starless core as mass becomes concentrated in the cen...
We present an Atacama Large Millimeter/submillimeter Array (ALMA) 106 GHz (Band 3) continuum survey ...
We present an Atacama Large Millimeter/submillimeter Array (ALMA) 106 GHz (Band 3) continuum survey ...
We present SMA and CARMA continuum and spectral line observations of five dense cores located in the...
The initial physical conditions of high-mass stars and protoclusters remain poorly characterized. To...
While clearly a vital step in the process of star formation, the transition from prestellar core to ...
Interpreting the nature of starless cores has been a prominent goal in star formation for many years...
The nearby Chamaeleon molecular cloud complex is a good laboratory to study the process of low-mass ...
Context. Chamaeleon I is the most active region in terms of star formation in the Chamaeleon molecul...
Chamaeleon I is the most active region in terms of star formation in the Chamaeleon molecular cloud ...
We present an unbiased census of starless cores in Perseus, Serpens, and Ophiuchus, assembled by com...
Although the standard model of star formation has served us well for over 20 years, its details are ...
In this paper, we present the results of a high resolution (5'') Combined Array for Research in Mill...