Mapping NGC 7027 in New Light: CO+ and HCO+ Emission Reveal Its Photon- and X-Ray-dominated Regions

The young and well-studied planetary nebula (PN) NGC 7027 harbors significant molecular gas that is irradiated by luminous, pointlike UV (central star) and diffuse (shocked nebular) X-ray emission. This nebula represents an excellent subject to investigate the molecular chemistry and physical condit...

Бүрэн тодорхойлолт

Номзүйн дэлгэрэнгүй

Үндсэн зохиолчид:	Jesse Bublitz, Joel H. Kastner, Pierre Hily-Blant, Thierry Forveille, Miguel Santander-García, Javier Alcolea, Valentin Bujarrabal, David J. Wilner, Rodolfo Montez Jr., Isabel Aleman
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	IOP Publishing 2022-01-01
Цуврал:	The Astrophysical Journal
Нөхцлүүд:	Astrochemistry Radio astronomy Planetary nebulae Bipolar nebulae Molecular gas
Онлайн хандалт:	https://doi.org/10.3847/1538-4357/aca405
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!