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Scattering-induced intensity reduction: large mass content with small grains in the inner region of...

Scattering-induced intensity reduction: large mass content with small grains in the inner region of...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2381870942

Scattering-induced intensity reduction: large mass content with small grains in the inner region of the TW Hya disk

About this item

Full title

Scattering-induced intensity reduction: large mass content with small grains in the inner region of the TW Hya disk

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2020-03

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Dust continuum observation is one of the best methods to constrain the properties of protoplanetary disks. Recent theoretical studies have suggested that the dust scattering at the millimeter wavelength potentially reduces the observed intensity, which results in an underestimate in the dust mass. We investigate whether the dust scattering indeed r...

Alternative Titles

Full title

Scattering-induced intensity reduction: large mass content with small grains in the inner region of the TW Hya disk

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2381870942

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2381870942

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2003.09353

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