GBT25A-448

CO observations of LHAASO J2002+3244u

Abstract

We plan to map the velocity and angular distribution of CO emission in a field around supernova remnant LHAASO J2002+3244u to determine if it is interacting with the radio supernova shell. If so, using the estimated density of any incident molecular clouds, we will be able to constrain the energy of hadronic cosmic rays produced by this supernova remnant.

Investigators

Name	Institution
Philip Lah *	Sydney, University of; Abu Dhabi, New York University
Joseph Gelfand	New York University; National Science Foundation ; Abu Dhabi, New York University
Moaz Abdelmaguid	New York University; Abu Dhabi, New York University
Jason Alford	Abu Dhabi, New York University
Kaya Mori	Columbia University
Naomi Tsuji	Tokyo, University of
Aya Bamba	Tokyo, University of

* indicates the PI