Chemical evolution of star-forming regions
EF Van Dishoeck, GA Blake - Annual Review of Astronomy and …, 1998 - annualreviews.org
▪ Abstract Recent advances in the understanding of the chemical processes that occur
during all stages of the formation of stars, from the collapse of molecular clouds to the …
during all stages of the formation of stars, from the collapse of molecular clouds to the …
Bipolar molecular outflows from young stars and protostars
R Bachiller - Annual Review of Astronomy and Astrophysics, 1996 - annualreviews.org
▪ Abstract A violent outflow of high-velocity gas is one of the first manifestations of the
formation of a new star. Such outflows emerge bipolarly from the young object and involve …
formation of a new star. Such outflows emerge bipolarly from the young object and involve …
Characterizing young protostellar disks with the CALYPSO IRAM-PdBI survey: large Class 0 disks are rare
Context. Understanding the formation mechanisms of protoplanetary disks and multiple
systems and also their pristine properties are key questions for modern astrophysics. The …
systems and also their pristine properties are key questions for modern astrophysics. The …
From Pre-stellar cores to protostars: The initial conditions of star formation
P Andre, D Ward-Thompson, M Barsony - arXiv preprint astro-ph/9903284, 1999 - arxiv.org
The last decade has witnessed significant advances in our observational understanding of
the earliest stages of low-mass star formation. The advent of sensitive receivers on large …
the earliest stages of low-mass star formation. The advent of sensitive receivers on large …
TADPOL: A 1.3 mm survey of dust polarization in star-forming cores and regions
We present λ 1.3 mm Combined Array for Research in Millimeter-wave Astronomy
observations of dust polarization toward 30 star-forming cores and eight star-forming regions …
observations of dust polarization toward 30 star-forming cores and eight star-forming regions …
Chemical evolution in preprotostellar and protostellar cores
EA Bergin, WD Langer - The Astrophysical Journal, 1997 - iopscience.iop.org
The chemistry of developing and collapsing low-mass protostellar cores is followed using a
chemical code with a time-varying density. Two evolutionary scenarios are represented …
chemical code with a time-varying density. Two evolutionary scenarios are represented …
Star formation in clusters: A survey of compact millimeter-wave sources in the Serpens core
L Testi, AI Sargent - The Astrophysical Journal, 1998 - iopscience.iop.org
We report the results of a millimeter interferometric survey of compact 3 mm continuum
sources in the inner 5 &farcm; 5× 5 &farcm; 5 region of the Serpens core. We detect 32 …
sources in the inner 5 &farcm; 5× 5 &farcm; 5 region of the Serpens core. We detect 32 …
The CALYPSO IRAM-PdBI survey of jets from Class 0 protostars-Exploring whether jets are ubiquitous in young stars
Aims. As a part of the CALYPSO Large Program, we aim to constrain the properties of
protostellar jets and outflows by searching for corresponding emission in a sample of 21 …
protostellar jets and outflows by searching for corresponding emission in a sample of 21 …
Low dust emissivities and radial variations in the envelopes of Class 0 protostars: possible signature of early grain growth
Context. Analyzing the properties of dust and its evolution in the early phases of star
formation is crucial to put constraints on the collapse and accretion processes as well as on …
formation is crucial to put constraints on the collapse and accretion processes as well as on …
[HTML][HTML] A molecular line study of NGC 1333/IRAS 4
GA Blake, G Sandell, EF Van Dishoeck… - … Journal, Part 1 …, 1995 - adsabs.harvard.edu
Molecular line surveys and fully sampled spectral line maps at 1.3 and 0.87 mm are used to
examine the physical and chemical characteristics of the extreme Class I sources IRAS 4A …
examine the physical and chemical characteristics of the extreme Class I sources IRAS 4A …