Add to ORKGThe 5 to 25 micron observations show that an object previously discovered at 2.2 microns (IRS 5) within the densest part of the L1551 dark cloud is a strong source of radiation from grains as cool as 230 K. The energy distribution resembles that of infrared objects embedded within other molecular cloud cores, but implies a total solar luminosity of only 30. The luminosity of the source and its proximity to other T Tauri stars suggests that it is a 1 to 2 solar mass pre-main sequence star still swaddled within the L1551 cloud. The radio and optical evidence for mass motions around IRS 5 may mean that IRS 5 has been flaring in FU Ori-type eruptions within the last 1000 years
XZ Tauri is a M3 V T Tauri star with a pre-main-sequence binary companion detected by infrared speck...
The L1551 molecular cloud contains two small clusters of Class 0 and I protostars, as well as a halo...
XZ Tauri is a M3 V T Tauri star with a pre-main-sequence binary companion detected by infrared speck...
Aims: The immediate vicinity of T Tauri was observed with the new high-contrast imaging instrument ...
We present the first Spitzer Infrared Spectrograph (IRS; The IRS was a collaborative venture between...
We have been surveying the Taurus dark cloud for young stars using a variety of techniques. Two opti...
Low mass pre-main sequence stars in the nearby Lynds 1551 star forming cloud are studied with the RO...
We present observations of several T Tauri stars using long baseline infrared interferometry from th...
We report observations of the T Tauri system at 8.4 GHz with a VLBI array comprising the VLBA, VLA a...
The Taurus molecular cloud supposedly has no star clusters but only isolated star formation. However...
We report the detection of quiescent H2 emission in the v=1→0 S(1) line at 2.12183 µm in the circums...
Planetary camera images of HL Tauri have been obtained through V-, R-, and I-band filters using the ...
We report the detection of quiescent H2 emission in the v 1! 0 S(1) line at 2.12183 lm in the circu...
Planetary camera images of HL Tauri have been obtained through V-, R-, and I-band filters using the ...
Infrared emission of circumstellar dust was observed for almost one hundred T Tauri stars. This dust...
XZ Tauri is a M3 V T Tauri star with a pre-main-sequence binary companion detected by infrared speck...
The L1551 molecular cloud contains two small clusters of Class 0 and I protostars, as well as a halo...
XZ Tauri is a M3 V T Tauri star with a pre-main-sequence binary companion detected by infrared speck...
Aims: The immediate vicinity of T Tauri was observed with the new high-contrast imaging instrument ...
We present the first Spitzer Infrared Spectrograph (IRS; The IRS was a collaborative venture between...
We have been surveying the Taurus dark cloud for young stars using a variety of techniques. Two opti...
Low mass pre-main sequence stars in the nearby Lynds 1551 star forming cloud are studied with the RO...
We present observations of several T Tauri stars using long baseline infrared interferometry from th...
We report observations of the T Tauri system at 8.4 GHz with a VLBI array comprising the VLBA, VLA a...
The Taurus molecular cloud supposedly has no star clusters but only isolated star formation. However...
We report the detection of quiescent H2 emission in the v=1→0 S(1) line at 2.12183 µm in the circums...
Planetary camera images of HL Tauri have been obtained through V-, R-, and I-band filters using the ...
We report the detection of quiescent H2 emission in the v 1! 0 S(1) line at 2.12183 lm in the circu...
Planetary camera images of HL Tauri have been obtained through V-, R-, and I-band filters using the ...
Infrared emission of circumstellar dust was observed for almost one hundred T Tauri stars. This dust...
XZ Tauri is a M3 V T Tauri star with a pre-main-sequence binary companion detected by infrared speck...
The L1551 molecular cloud contains two small clusters of Class 0 and I protostars, as well as a halo...
XZ Tauri is a M3 V T Tauri star with a pre-main-sequence binary companion detected by infrared speck...