806 citations · 8k across the 121 of their papers we have counts for
7 papers · 2 filters
Outflows, Accretion, and Clustered Protostellar Cores around a Forming O Star
Keping Qiu, Qizhou Zhang, Karl M. Menten
We present a Submillimeter Array study in the 1.3 mm waveband of the NGC 7538 IRS 1--3 massive star-forming region. The brightest core in the mm continuum map, MM1, harbors the IRS…
The magnetic field in the NGC 2024 FIR 5 dense core
Felipe de O. Alves, Josep M. Girart, Shih-Ping Lai +2
We used the Submillimeter Array (SMA) to observe the thermal polarized dust emission from the protostellar source NGC 2024 FIR 5. The polarized emission outlines a partial hourglas…
IRAS 22198+6336: Discovery of an Intermediate-Mass Hot Core
Alvaro Sanchez-Monge, Aina Palau, Robert Estalella +4
We present new SMA and PdBI observations of the intermediate-mass object IRAS 22198+6336 in the millimeter continuum and in several molecular line transitions. The millimeter conti…
Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way
S. Molinari, B. Swinyard, J. Bally +121
We present the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key-project that will map the inner Galactic Plane of the Milky Way in 5 bands…
From the Convergence of Filaments to Disk-Outflow Accretion: Massive-Star Formation in W33A
Roberto Galván-Madrid, Qizhou Zhang, Eric Keto +5
Interferometric observations of the W33A massive star-formation region, performed with the Submillimeter Array (SMA) and the Very Large Array (VLA) at resolutions from 5 arcsec (0.…
The standard model of star formation applied to massive stars: accretion disks and envelopes in molecular lines
Eric Keto, Qizhou Zhang
We address the question of whether the formation of high-mass stars is similar to or differs from that of solar-mass stars through new molecular line observations and modeling of t…
The reflection-symmetric wiggle of the young protostellar jet HH 211
Chin-Fei Lee, Tatsuhiko I. Hasegawa, Naomi Hirano +4
HH 211 is a highly collimated jet originating from a nearby young Class 0 protostar. Here is a follow-up study of the jet with our previous observations at unprecedented resolution…