The UV Perspective of Low-Mass Star Formation

The formation of low-mass (<inline-formula> <math display="inline"> <semantics> <mrow> <msub> <mi>M</mi> <mo>★</mo> </msub> <mo>≲</mo> <mn>2</mn> <mspace width="0.166667em"></mspace> &...

Full description

Bibliographic Details
Main Authors: P. Christian Schneider, H. Moritz Günther, Kevin France
Format: Article
Language:English
Published: MDPI AG 2020-03-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/8/1/27
_version_ 1819012478337548288
author P. Christian Schneider
H. Moritz Günther
Kevin France
author_facet P. Christian Schneider
H. Moritz Günther
Kevin France
author_sort P. Christian Schneider
collection DOAJ
description The formation of low-mass (<inline-formula> <math display="inline"> <semantics> <mrow> <msub> <mi>M</mi> <mo>★</mo> </msub> <mo>≲</mo> <mn>2</mn> <mspace width="0.166667em"></mspace> <msub> <mi>M</mi> <mo>⊙</mo> </msub> </mrow> </semantics> </math> </inline-formula>) stars in molecular clouds involves accretion disks and jets, which are of broad astrophysical interest. Accreting stars represent the closest examples of these phenomena. Star and planet formation are also intimately connected, setting the starting point for planetary systems like our own. The ultraviolet (UV) spectral range is particularly suited for studying star formation, because virtually all relevant processes radiate at temperatures associated with UV emission processes or have strong observational signatures in the UV range. In this review, we describe how UV observations provide unique diagnostics for the accretion process, the physical properties of the protoplanetary disk, and jets and outflows.
first_indexed 2024-12-21T01:44:41Z
format Article
id doaj.art-c79d407bdbbf4e3090f2a5cd313d3cc9
institution Directory Open Access Journal
issn 2075-4434
language English
last_indexed 2024-12-21T01:44:41Z
publishDate 2020-03-01
publisher MDPI AG
record_format Article
series Galaxies
spelling doaj.art-c79d407bdbbf4e3090f2a5cd313d3cc92022-12-21T19:20:03ZengMDPI AGGalaxies2075-44342020-03-01812710.3390/galaxies8010027galaxies8010027The UV Perspective of Low-Mass Star FormationP. Christian Schneider0H. Moritz Günther1Kevin France2Hamburger Sternwarte, University of Hamburg, 21029 Hamburg, GermanyMassachusetts Institute of Technology, Kavli Institute for Astrophysics and Space Research; Cambridge, MA 02109, USADepartment of Astrophysical and Planetary Sciences Laboratory for Atmospheric and Space Physics, University of Colorado, Denver, CO 80203, USAThe formation of low-mass (<inline-formula> <math display="inline"> <semantics> <mrow> <msub> <mi>M</mi> <mo>★</mo> </msub> <mo>≲</mo> <mn>2</mn> <mspace width="0.166667em"></mspace> <msub> <mi>M</mi> <mo>⊙</mo> </msub> </mrow> </semantics> </math> </inline-formula>) stars in molecular clouds involves accretion disks and jets, which are of broad astrophysical interest. Accreting stars represent the closest examples of these phenomena. Star and planet formation are also intimately connected, setting the starting point for planetary systems like our own. The ultraviolet (UV) spectral range is particularly suited for studying star formation, because virtually all relevant processes radiate at temperatures associated with UV emission processes or have strong observational signatures in the UV range. In this review, we describe how UV observations provide unique diagnostics for the accretion process, the physical properties of the protoplanetary disk, and jets and outflows.https://www.mdpi.com/2075-4434/8/1/27star formationultravioletlow-mass stars
spellingShingle P. Christian Schneider
H. Moritz Günther
Kevin France
The UV Perspective of Low-Mass Star Formation
Galaxies
star formation
ultraviolet
low-mass stars
title The UV Perspective of Low-Mass Star Formation
title_full The UV Perspective of Low-Mass Star Formation
title_fullStr The UV Perspective of Low-Mass Star Formation
title_full_unstemmed The UV Perspective of Low-Mass Star Formation
title_short The UV Perspective of Low-Mass Star Formation
title_sort uv perspective of low mass star formation
topic star formation
ultraviolet
low-mass stars
url https://www.mdpi.com/2075-4434/8/1/27
work_keys_str_mv AT pchristianschneider theuvperspectiveoflowmassstarformation
AT hmoritzgunther theuvperspectiveoflowmassstarformation
AT kevinfrance theuvperspectiveoflowmassstarformation
AT pchristianschneider uvperspectiveoflowmassstarformation
AT hmoritzgunther uvperspectiveoflowmassstarformation
AT kevinfrance uvperspectiveoflowmassstarformation