Toward the identification of cyano-astroCOMs via vibrational features: benzonitrile as a test case. [PDF]
Xu Y, Biczysko M.
europepmc +1 more source
Astrochemical evolution along star formation: Overview of the IRAM Large Program ASAI. [PDF]
Lefloch B +29 more
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Chemical segregation in the young protostars Barnard 1b-N and S Evidence of pseudo-disk rotation in Barnard 1b-S. [PDF]
Fuente A +9 more
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Comprehensive Atomistic Simulations of Fischer-Tropsch in Outer Space: Astrocatalysis by Fe<sub>13</sub>-Supported Nanoclusters on SiO<sub>2</sub>. [PDF]
Pareras G +3 more
europepmc +1 more source
Microwave Receiving System Based on Cryogenic Sensors for the Optical Big Telescope Alt-Azimuth. [PDF]
Balega Y +21 more
europepmc +1 more source
Magnetic fields of low-mass stars & protostars. Observations & results
Magnetic field are ubiquitous to young and mature low-mass stars, and can potentially impact their formation, their evolution and their internal structure; yet the physical processes that succeed at amplifying and sustaining these fields (called dynamo processes), like those capable of changing the fate of the host stars (and in particular their ...
J.-F. Donati
openaire +2 more sources
Optical spectroscopy of Gaia detected protostars with DOT: Can we probe protostellar photospheres?
Optical spectroscopy offers the most direct view of the stellar properties and the accretion indicators. Standard accretion tracers, such as $H\beta$, $H\alpha$, and, Ca II triplet lines, and most photospheric features, fall in the optical wavelengths ...
Mayank Narang +2 more
exaly +4 more sources
Related searches:
NGC 1333—Protostars, Dust Shells, and Triggered Star Formation
The Astrophysical Journal, 2001We present large (13' × 18') and sensitive continuum maps at 850 and 450 μm of the NGC 1333 star formation region. We identify 33 submillimeter sources, some of which are extended and may contain multiple condensations. Very few of the submillimeter sources have optical or near-IR counterparts. In addition to the previously known bright class 0 sources,
Göran Sandell, Lewis B. G. Knee
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