International audienceWe present a new millimeter survey of 23 pre-main-sequence stars in the Taurus-Auriga star-forming region. The main goal of the project was to identify circumstellar disks around stars of late spectral types (M * lsim 0.7 M sun). We used the IRAM Plateau de Bure Interferometer to obtain observations at 1.3 mm, 2.7 mm, and the CO J = 1-0 and J = 2-1 lines. We detected eight sources in continuum emission, with new detections of CIDA-1 and CIDA-8 at 1.3 mm. Overall, we find that circumstellar disks around stars with spectral types later than M2 tend to have smaller millimeter continuum fluxes than those around earlier type stars. We also present four detections of disks in their CO line emission (LkHα 358, GO Tau, Haro 6-...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
Four Ophiuchus binaries, two Class I systems and two Class II systems, with separations of similar t...
We present a new millimeter survey of 23 pre-main-sequence stars in the Taurus-Auriga star-forming r...
We present millimeter-wave continuum images of four wide (separations 210-800 AU) young stellar bina...
We have used the high sensitivity and resolution of the IRAM interferometer to produce sub-arcsecond...
The results of a combined millimeter-spectral-line and continuum survey of cold far-infrared sources...
The structure and composition of circumstellar disks around young stars is one of the areas in which...
We present millimeter-wave continuum images of four wide (separations 210-800 AU), young stellar bin...
We have conducted a survey of 17 wide (〉100 AU) young binary systems in Taurus with the Atacama Larg...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
There is now a substantial body of evidence that disk-like structures of gas and dust surround many ...
Four Ophiuchus binaries, two Class I systems and two Class II systems, with separations of similar t...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
Four Ophiuchus binaries, two Class I systems and two Class II systems, with separations of similar t...
We present a new millimeter survey of 23 pre-main-sequence stars in the Taurus-Auriga star-forming r...
We present millimeter-wave continuum images of four wide (separations 210-800 AU) young stellar bina...
We have used the high sensitivity and resolution of the IRAM interferometer to produce sub-arcsecond...
The results of a combined millimeter-spectral-line and continuum survey of cold far-infrared sources...
The structure and composition of circumstellar disks around young stars is one of the areas in which...
We present millimeter-wave continuum images of four wide (separations 210-800 AU), young stellar bin...
We have conducted a survey of 17 wide (〉100 AU) young binary systems in Taurus with the Atacama Larg...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
There is now a substantial body of evidence that disk-like structures of gas and dust surround many ...
Four Ophiuchus binaries, two Class I systems and two Class II systems, with separations of similar t...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
We have conducted a survey of young single and multiple systems in the Taurus–Auriga star-forming re...
Four Ophiuchus binaries, two Class I systems and two Class II systems, with separations of similar t...