Microarcsecond radio astrometry
MJ Reid, M Honma - Annual Review of Astronomy and …, 2014 - annualreviews.org
Astrometry provides the foundation for astrophysics. Accurate positions are required for the
association of sources detected at different times or wavelengths, and distances are …
association of sources detected at different times or wavelengths, and distances are …
Warm carbon-chain chemistry
N Sakai, S Yamamoto - Chemical Reviews, 2013 - ACS Publications
1.1. Interstellar Clouds and Interstellar Chemistry A space between stars is not completely a
vacuum, but is filled up with interstellar gas, whose average number density of H nuclei in all …
vacuum, but is filled up with interstellar gas, whose average number density of H nuclei in all …
Probing the evolution of molecular cloud structure-From quiescence to birth
J Kainulainen, H Beuther, T Henning… - Astronomy & …, 2009 - aanda.org
Context. Probability distribution of densities is a fundamental measure of molecular cloud
structure, containing information on how the material arranges itself in molecular clouds …
structure, containing information on how the material arranges itself in molecular clouds …
Change in the chemical composition of infalling gas forming a disk around a protostar
N Sakai, T Sakai, T Hirota, Y Watanabe, C Ceccarelli… - Nature, 2014 - nature.com
Abstract IRAS 04368+ 2557 is a solar-type (low-mass) protostar embedded in a protostellar
core (L1527) in the Taurus molecular cloud,, which is only 140 parsecs away from Earth …
core (L1527) in the Taurus molecular cloud,, which is only 140 parsecs away from Earth …
Mapping the shores of the Brown Dwarf desert. II. Multiple star formation in Taurus–Auriga
We have conducted a high-resolution imaging study of the Taurus–Auriga star-forming
region in order to characterize the primordial outcome of multiple star formation and the …
region in order to characterize the primordial outcome of multiple star formation and the …
Structure and kinematics of the Taurus star-forming region from Gaia-DR2 and VLBI astrometry
Aims. We take advantage of the second data release of the Gaia space mission and the
state-of-the-art astrometry delivered from very long baseline interferometry observations to …
state-of-the-art astrometry delivered from very long baseline interferometry observations to …
The stellar membership of the taurus star-forming region
KL Luhman - The Astronomical Journal, 2018 - iopscience.iop.org
The high-precision astrometry from the second data release of the Gaia mission has made it
possible to greatly improve the census of members of nearby clusters and associations. I …
possible to greatly improve the census of members of nearby clusters and associations. I …
The Gould's Belt Distances Survey (GOBELINS). I. Trigonometric parallax distances and depth of the ophiuchus complex
We present the first results of the Gould's Belt Distances Survey (GOBELINS), a project
aimed at measuring the proper motion and trigonometric parallax of a large sample of young …
aimed at measuring the proper motion and trigonometric parallax of a large sample of young …
BANYAN. VII. A new population of young substellar candidate members of nearby moving groups from the BASS survey
We present the results of a near-infrared (NIR) spectroscopic follow-up survey of 182 M4–L7
low-mass stars and brown dwarfs (BDs) from the BANYAN All-Sky Survey (BASS) for …
low-mass stars and brown dwarfs (BDs) from the BANYAN All-Sky Survey (BASS) for …
Precision timing of PSR J0437–4715: an accurate pulsar distance, a high pulsar mass, and a limit on the variation of Newton's gravitational constant
Analysis of 10 years of high-precision timing data on the millisecond pulsar PSR J0437–
4715 has resulted in a model-independent kinematic distance based on an apparent orbital …
4715 has resulted in a model-independent kinematic distance based on an apparent orbital …