Interferometric studies of low-mass protostars

Publikation: Bidrag til bog/antologi/rapport › Konferencebidrag i proceedings › Forskning › fagfællebedømt

Standard

Interferometric studies of low-mass protostars. / Jørgensen, Jes K.

The Molecular Universe. red. / Jose Cernicharo; Rafael Madrid. S280. udg. 2011. s. 53-64 (Proceedings of the International Astronomical Union; Nr. S280, Bind 7).

Publikation: Bidrag til bog/antologi/rapport › Konferencebidrag i proceedings › Forskning › fagfællebedømt

Harvard

Jørgensen, JK 2011, Interferometric studies of low-mass protostars. i J Cernicharo & R Madrid (red), The Molecular Universe. S280 udg, Proceedings of the International Astronomical Union, nr. S280, bind 7, s. 53-64. https://doi.org/10.1017/S1743921311024860

APA

Jørgensen, J. K. (2011). Interferometric studies of low-mass protostars. I J. Cernicharo, & R. Madrid (red.), The Molecular Universe (S280 udg., s. 53-64). Proceedings of the International Astronomical Union Bind 7 Nr. S280 https://doi.org/10.1017/S1743921311024860

Vancouver

Jørgensen JK. Interferometric studies of low-mass protostars. I Cernicharo J, Madrid R, red., The Molecular Universe. S280 udg. 2011. s. 53-64. (Proceedings of the International Astronomical Union; Nr. S280, Bind 7). https://doi.org/10.1017/S1743921311024860

Author

Jørgensen, Jes K. / Interferometric studies of low-mass protostars. The Molecular Universe. red. / Jose Cernicharo ; Rafael Madrid. S280. udg. 2011. s. 53-64 (Proceedings of the International Astronomical Union; Nr. S280, Bind 7).

Bibtex

@inproceedings{de0d278312d94328ae6ebb462605683e,
title = "Interferometric studies of low-mass protostars",
abstract = "With the advances in high angular resolution (sub)millimeter observations of lowmass protostars, windows of opportunities are opening up for very detailed studies of the molecular structure of star forming regions on wide range of spatial scales. Deeply embedded protostars provide an important laboratory to study the chemistry of star formation-providing the link between dense regions in molecular clouds from which stars are formed, i.e., the initial conditions and the end product in terms of, e.g., disk and planet formation. High angular resolution observations at (sub)millimeter wavelengths provide an important tool for studying the chemical composition of such low-mass protostars. They for example constrain the spatial molecular abundance variations-and can thereby identify which species are useful tracers of different components of the protostars at different evolutionary stages. In this review I discuss the possibilities and limitations of using high angular resolution (sub)millimeter interferometric observations for studying the chemical evolution of low-mass protostars-with a particular keen eye toward near-future ALMA observations.",
keywords = "Astrochemistry, ISM: abundances, ISM: molecules, Planetary systems: protoplanetary disks, Radiative transfer, Stars: formation, Techniques: high angular resolution, Techniques: interferometric",
author = "J{\o}rgensen, {Jes K.}",
year = "2011",
month = jun,
day = "1",
doi = "10.1017/S1743921311024860",
language = "English",
isbn = "9781107019805",
series = "Proceedings of the International Astronomical Union",
publisher = "Cambridge University Press",
number = "S280",
pages = "53--64",
editor = "Jose Cernicharo and Rafael Madrid",
booktitle = "The Molecular Universe",
edition = "S280",

}

RIS

TY - GEN

T1 - Interferometric studies of low-mass protostars

AU - Jørgensen, Jes K.

PY - 2011/6/1

Y1 - 2011/6/1

N2 - With the advances in high angular resolution (sub)millimeter observations of lowmass protostars, windows of opportunities are opening up for very detailed studies of the molecular structure of star forming regions on wide range of spatial scales. Deeply embedded protostars provide an important laboratory to study the chemistry of star formation-providing the link between dense regions in molecular clouds from which stars are formed, i.e., the initial conditions and the end product in terms of, e.g., disk and planet formation. High angular resolution observations at (sub)millimeter wavelengths provide an important tool for studying the chemical composition of such low-mass protostars. They for example constrain the spatial molecular abundance variations-and can thereby identify which species are useful tracers of different components of the protostars at different evolutionary stages. In this review I discuss the possibilities and limitations of using high angular resolution (sub)millimeter interferometric observations for studying the chemical evolution of low-mass protostars-with a particular keen eye toward near-future ALMA observations.

AB - With the advances in high angular resolution (sub)millimeter observations of lowmass protostars, windows of opportunities are opening up for very detailed studies of the molecular structure of star forming regions on wide range of spatial scales. Deeply embedded protostars provide an important laboratory to study the chemistry of star formation-providing the link between dense regions in molecular clouds from which stars are formed, i.e., the initial conditions and the end product in terms of, e.g., disk and planet formation. High angular resolution observations at (sub)millimeter wavelengths provide an important tool for studying the chemical composition of such low-mass protostars. They for example constrain the spatial molecular abundance variations-and can thereby identify which species are useful tracers of different components of the protostars at different evolutionary stages. In this review I discuss the possibilities and limitations of using high angular resolution (sub)millimeter interferometric observations for studying the chemical evolution of low-mass protostars-with a particular keen eye toward near-future ALMA observations.

KW - Astrochemistry

KW - ISM: abundances

KW - ISM: molecules

KW - Planetary systems: protoplanetary disks

KW - Radiative transfer

KW - Stars: formation

KW - Techniques: high angular resolution

KW - Techniques: interferometric

UR - http://www.scopus.com/inward/record.url?scp=84882755055&partnerID=8YFLogxK

U2 - 10.1017/S1743921311024860

DO - 10.1017/S1743921311024860

M3 - Article in proceedings

AN - SCOPUS:84882755055

SN - 9781107019805

T3 - Proceedings of the International Astronomical Union

SP - 53

EP - 64

BT - The Molecular Universe

A2 - Cernicharo, Jose

A2 - Madrid, Rafael

ER -

ID: 229737291