27 citations · 128 across the 12 of their papers we have counts for
7 papers · 1 filter
Loose threads: parsec-scale filamentation in the high Galactic latitude molecular clouds MBM 3 and MBM 16
Marco Monaci, Loris Magnani, Steven N. Shore
The existence of high galactic latitude molecular clouds has been known for several decades, and studies of their dust and gas distributions reveal complicated morphological struct…
Shear, writhe and filaments: turbulence in the high latitude molecular cloud MBM 40
Marco Monaci, Loris Magnani, Steven N. Shore +2
Context. It is almost banal to say that the interstellar medium (ISM) is structurally and thermodynamically complex. But the variety of the governing processes, including stellar f…
The mixing of dust and gas in the high latitude translucent cloud MBM 40
Marco Monaci, Loris Magnani, Steven N. Shore
Context. High latitude molecular clouds (hereafter HLMCs) permit the study of interstellar gas dynamics and astrochemistry with good accuracy due to their proximity, generally clea…
Sensitive CO(1-0) Survey in Pegasus-Pisces Reduces CO-Dark Gas Inventory by Factor of Two
Emmanuel Donate, Loris Magnani
We conducted high-sensitivity, high-velocity resolution CO(1-0) observations in a region containing a portion of the diffuse molecular cloud MBM 53 to determine whether weak CO emi…
A High-Resolution Study of the CO-H2 Conversion Factor in the Diffuse Cloud MBM 40
David L. Cotten, Loris Magnani
We made CO(1-0) observations of 103 lines of sight in the core and envelope of the high-latitude cloud MBM 40 to determine how the CO-H_2 conversion factor (X_CO) varies throughout…
Molecular gas and stars in the translucent cloud MBM 18 (LDN 1569)
J. Brand, J. G. A. Wouterloot, L. Magnani
Seven of ten candidate H-alpha emission-line stars found in an objective grism survey of a 1 square degree region in MBM 18, were observed spectroscopically. Four of these have wea…
Hydroxyl as a Tracer of H2 in the Envelope of MBM40
David L. Cotten, Loris Magnani, Elizabeth A. Wennerstrom +2
We observed 51 positions in the OH 1667 MHz main line transitions in the translucent, high latitude cloud MBM40. We detected OH emission in 8 out of 8 positions in the molecular co…