Aperture Synthesis C18O (1-0) Observations of L 1551 IRS5
M Munetake, O Nagayoshi, K Ryohei… - … Astrophysics in Asia …, 1999 - ui.adsabs.harvard.edu
We report aperture synthesis jceto observations of L1551 IRS5 with a spatial resolution of
2.8" x 2.5" using the Nobeyama Millimeter Array. We have detected an emission component …
2.8" x 2.5" using the Nobeyama Millimeter Array. We have detected an emission component …
Aperture Synthesis C18O J= 1-0 Observations of L1551 IRS 5: Detailed Structure of the Infalling Envelope
We report aperture synthesis C 18 OJ= 1–0 observations of L1551 IRS 5 with a spatial
resolution of 2 &farcs; 8× 2 &farcs; 5 using the Nobeyama Millimeter Array. We have …
resolution of 2 &farcs; 8× 2 &farcs; 5 using the Nobeyama Millimeter Array. We have …
[HTML][HTML] High Resolution Imaging of the Protostellar Envelope around L1551 IRS 5: Growth of the Circumstellar Disk
M Momose - Star Formation 1999, 1999 - adsabs.harvard.edu
We report aperture synthesis C 18 O (J= 1-0) observations of L1551 IRS 5 with a spatial
resolution of 2.8''x 2.5''using the Nobeyama Millimeter Array. We have detected an emission …
resolution of 2.8''x 2.5''using the Nobeyama Millimeter Array. We have detected an emission …
Imaging of an infalling disklike envelope around L1551 IRS 5
M Saito, R Kawabe, Y Kitamura… - The Astrophysical …, 1996 - iopscience.iop.org
Aperture synthesis observations of H13CO(J\1» 0) emission from L1551 IRS 5 were made
using the Nobeyama Millimeter Array. It is found that the emission has a disklike structure …
using the Nobeyama Millimeter Array. It is found that the emission has a disklike structure …
A 45 AU radius source around L1551-IRS 5: a possible accretion disk
J Keene, CR Masson - Symposium-International Astronomical Union, 1991 - cambridge.org
Our interferometric and single-dish observations of the continuum emission from L1551-IRS
5 show that, at millimeter wavelengths, there are two distinct components to the source, an …
5 show that, at millimeter wavelengths, there are two distinct components to the source, an …
[HTML][HTML] Spatially resolved submillimeter continuum emission toward L1551 IRS 5
We present high signal-to-noise ratio 16-20 arcsec resolution submillimeter continuum
images of the embedded young stellar object L1551 IRS 5. The images are dominated by a …
images of the embedded young stellar object L1551 IRS 5. The images are dominated by a …
Properties and formation of the multiple protostellar system L1551 IRS 5
J Lim, S Takakuwa - The Astrophysical Journal, 2006 - iopscience.iop.org
We present an observation of L1551 IRS 5 at 7 mm with an angular resolution as high as~ 0
farcs 04 (5 AU). Apart from the two main components oriented north-south with a projected …
farcs 04 (5 AU). Apart from the two main components oriented north-south with a projected …
[HTML][HTML] The Circumstellar Structure of Lynds 379 IRS 1
ML Kelly, GH Macdonald - … Space Science, Volume 224, Issue 1 …, 1995 - adsabs.harvard.edu
Abstract 12 CO J= 2-1 maps of L379 IRS1 show a molecular outflow seen almost end-on
while C 18 OJ= 2-1 emission covers a smaller central region, tracing virially bound material …
while C 18 OJ= 2-1 emission covers a smaller central region, tracing virially bound material …
[HTML][HTML] Possible Infall in the Gas Disk around L1551 IRS 5
N Ohashi, M Hayashi, PTP Ho… - … Journal v. 466, p …, 1996 - adsabs.harvard.edu
Possible Infall in the Gas Disk around L1551 IRS 5 ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …
completely retired in October 2019. This page will automatically redirect to the new ADS …
High resolution 2.7 mm observations of L1551 IRS5: A protobinary system?
We present sub-arcsecond resolution imaging of the λ= 2.7 mm continuum emission from
the young, embedded system L1551 IRS5 using the new, nine element, high resolution …
the young, embedded system L1551 IRS5 using the new, nine element, high resolution …