309 citations
- Center for Astrophysics Harvard & SmithsonianUS9 papers
- University of Illinois Urbana-ChampaignUS7 papers
- University of VirginiaUS7 papers
- Pennsylvania State UniversityUS6 papers
- Space Telescope Science InstituteUS6 papers
- Université Bourgogne Franche-ComtéFR6 papers
- University College LondonGB6 papers
- Carnegie Mellon UniversityUS5 papers
- Georgia State UniversityUS5 papers
- Ohio UniversityUS5 papers
- Seoul National UniversityKR5 papers
- Tel Aviv UniversityIL5 papers
13 papers · 1 filter
Absorption and Self-Absorption of [C II] and [O I] Far Infrared Lines Towards a Bright Bubble in the Nessie Infrared Dark Cloud
J. M. Jackson, J. S. Whitaker, E. T. Chambers +15
Using the upGREAT instrument on SOFIA, we have imaged [C II] 157.74 and [O I] 63.18 micron line emission from a bright photodissociation region (PDR) associated with an ionized ``b…
Can Protostellar Outflows Set Stellar Masses?
Philip C. Myers, Michael M. Dunham, Ian W. Stephens
The opening angles of some protostellar outflows appear too narrow to match the expected core-star mass efficiency SFE = 0.3-0.5 if outflow cavity volume traces outflow mass, with…
First BISTRO observations of the dark cloud Taurus L1495A-B10: the role of the magnetic field in the earliest stages of low-mass star formation
Derek Ward-Thompson, Janik Karoly, Kate Pattle +155
We present BISTRO Survey 850 μm dust emission polarisation observations of the L1495A-B10 region of the Taurus molecular cloud, taken at the JCMT. We observe a roughly triangular n…
The JCMT BISTRO Survey: Multi-wavelength polarimetry of bright regions in NGC 2071 in the far-infrared/submillimetre range, with POL-2 and HAWC+
L. Fanciullo, F. Kemper, K. Pattle +31
Polarized dust emission is a key tracer in the study of interstellar medium and of star formation. The observed polarization, however, is a product of magnetic field structure, dus…
The Magnetic Field in the Milky Way Filamentary Bone G47
Ian W. Stephens, Philip C. Myers, Catherine Zucker +21
Star formation primarily occurs in filaments where magnetic fields are expected to be dynamically important. The largest and densest filaments trace spiral structure within galaxie…
Evolution and Kinematics of Protostellar Envelopes in the Perseus Molecular Cloud
Daniel J. Heimsoth, Ian W. Stephens, Hector G. Arce +3
We present a comprehensive analysis on the evolution of envelopes surrounding protostellar systems in the Perseus molecular cloud using data from the MASSES survey. We focus our at…