The maser source S140-H2O as a protoplanetary disk
- 1 February 2001
- journal article
- Published by Pleiades Publishing Ltd in Astronomy Reports
- Vol. 45 (2) , 113-119
- https://doi.org/10.1134/1.1346720
Abstract
We present the observations of the H2O maser in S140 with the 22-m radio telescope of the Pushchino Radio Astronomy Observatory in 1992–1999. The H2O maser emission is mainly concentrated in three symKeywords
This publication has 7 references indexed in Scilit:
- Radio Continuum–H2O Maser Systems in NGC 2071: H2O Masers Tracing a Jet (IRS 1) and a Rotating Proto–Planetary Disk of Radius 20 AU (IRS 3)The Astrophysical Journal, 1998
- A Radio Jet–H2O Maser System in W75N(B) at a 200 Au Scale: Exploring the Evolutionary Stages of Young Stellar ObjectsThe Astrophysical Journal, 1997
- Ultracompact H II regions. 2: New high-resolution radio imagesThe Astrophysical Journal Supplement Series, 1994
- Infrared line and radio continuum emission of circumstellar ionized regionsThe Astrophysical Journal, 1983
- On the morphology of galaxies in clustersThe Astronomical Journal, 1980
- New multiple systems in molecular cloudsThe Astrophysical Journal, 1979
- The energetics of molecular clouds. II - The S140 molecular cloudThe Astrophysical Journal, 1978