Discovery of a Highly Collimated Flow from the High-mass Protostar ISOSS J23053+5953 SMM2
Tatiana M. Rodríguez(New Mexico Institute of Mining and Technology), Viviana Rosero(National Radio Astronomy Observatory), E. D. Araya(Western Illinois University), P. Höfner(New Mexico Institute of Mining and Technology), H. Linz(Max Planck Institute for Astronomy), S. Kurtz(Universidad Nacional Autónoma de México), Laura Gómez(Australian Carbon Innovation), Qizhou Zhang(Center for Astrophysics Harvard & Smithsonian), Carlos Carrasco‐González(Universidad Nacional Autónoma de México)
Cited by 5
Related Papers
Molecular gas kinematics within the central 250 pc of the Milky Way
|Monthly Notices of the Royal Astronomical Society|2016|229
Large Interferometer For Exoplanets (LIFE)
|Astronomy and Astrophysics|2022|187
Size controlled green synthesis of gold nanoparticles using <i>Coffea arabica</i> seed extract and their catalytic performance in 4-nitrophenol reduction
|RSC Advances|2018|117
Gravity or turbulence? – III. Evidence of pure thermal Jeans fragmentation at ∼0.1 pc scale
|Monthly Notices of the Royal Astronomical Society|2015|116
Monitoring the Large Proper Motions of Radio Sources in the Orion BN/KL Region
|The Astrophysical Journal|2008|107