Observations of 11 protostellar sources in Taurus with Nobeyama millimeter array-Growth of circumstellar disks

N Ohashi, R Kawabe, M Hayashi… - … Journal (ISSN 0004 …, 1991 - adsabs.harvard.edu
Results are presented of observations of the CS (J= 2-1) line and 98-GHz continua of 11
protostellar IRAS sources made with high spatial resolution of 2.8-8.8 arcsec using the …

[HTML][HTML] The Nobeyama Millimeter Array survey of young stellar objects associated with the Taurus molecular cloud

N Ohashi, M Hayashi, R Kawabe… - Astrophysical Journal v …, 1996 - adsabs.harvard.edu
We have carried out an interferometric survey of 3 mm continuum and CS (J= 2-1) line
emissions from 13 optically invisible protostar candidates and six young T Tauri stars …

On the origin of submillimeter emission from young stars in Taurus-Auriga

M Barsony, SJ Kenyon - … Journal, Part 2-Letters (ISSN 0004 …, 1992 - adsabs.harvard.edu
Submillimeter photometry of embedded sources in the nearby Taurus-Auriga molecular
cloud is presented. The submillimeter emission is found to contribute 5 percent or less to the …

Near-infrared and optical observations of IRAS sources in and near dense cores

PC Myers, GA Fuller, RD Mathieu… - … Journal, Part 1 …, 1987 - adsabs.harvard.edu
The authors report photometry from 0.4 to 20 μm of 34 IRAS point sources associated with
dense cores in dark clouds. The main results of this study are:(1) Stars near cores tend to be …

[HTML][HTML] Partial aperture synthesis of five dark clouds at 1.4 GHz

E Falgarone, W Gilmore - … and Astrophysics, vol. 95, no. 1, Feb …, 1981 - adsabs.harvard.edu
The paper reports 1.4 GHz continuum observations of five dark cloud regions using the
Westerbork Synthesis Radio Telescope. A total of 97 radio continuum sources were …

[HTML][HTML] Results of a radio survey for new compact H II regions

JE Wink, WJ Altenhoff… - … , vol. 108, no. 2, Apr. 1982 …, 1982 - adsabs.harvard.edu
Ninety-one sources that appeared to be point sources when observed with the angular
resolution of the 100-m telescope at 4.9 GHz, and that were expected to be H II regions …

[HTML][HTML] Millimeter and submillimeter wavelength continuum observations of massive young stellar objects

WH McCutcheon, T Sato, CR Purton… - … Journal v. 110, p …, 1995 - adsabs.harvard.edu
Millimeter and Submillimeter Wavelength Continuum Observations of Massive Young ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …

Optical veiling, disk accretion, and the evolution of T Tauri stars

LW Hartmann, SJ Kenyon - … Journal, Part 1 (ISSN 0004-637X) …, 1990 - adsabs.harvard.edu
High-resolution spectra of 31 K7-M1 T Tauri stars (TTs) in the Taurus-Auriga molecular
cloud demonstrate that most of these objects exhibit substantial excess emission at 5200 A …

[HTML][HTML] 1.3 mm continuum emission from circumstellar envelopes

CM Walmsley, R Chini, E Kreysa… - … (ISSN 0004-6361) …, 1991 - adsabs.harvard.edu
Abstract The 1.3-mm continuum emission from the circumstellar envelopes of late-type stars
are surveyed using both the IRAM 30-m (MRT) and SEST 15-m telescopes. Thirty-three late …

A survey for circumstellar disks around young stellar objects

SVW Beckwith, AI Sargent, RS Chini… - … Journal (ISSN 0004 …, 1990 - adsabs.harvard.edu
Continuum observations at 1.3 mm of 86 pre-main sequence stars in the Taurus-Auriga dark
clouds show that 42% have detectable emission from small particles. The detected fraction …