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The Astrophysical Journal Supplement (ApJS)

Resumen/Descripción – provisto por la editorial en inglés
The Astrophysical Journal Supplement is an open access journal publishing significant articles containing extensive data or calculations. ApJS also supports Special Issues, collections of thematically related papers published simultaneously in a single volume.
Palabras clave – provistas por la editorial

astronomy; astrophysics

Disponibilidad
Institución detectada Período Navegá Descargá Solicitá
No detectada desde dic. 1996 / hasta dic. 2023 IOPScience

Información

Tipo de recurso:

revistas

ISSN impreso

0067-0049

ISSN electrónico

1538-4365

Editor responsable

American Astronomical Society (AAS)

Idiomas de la publicación

  • inglés

País de edición

Reino Unido

Información sobre licencias CC

https://creativecommons.org/licenses/by/4.0/

Cobertura temática

Tabla de contenidos

Molecules with ALMA at Planet-forming Scales (MAPS). V. CO Gas Distributions

Ke ZhangORCID; Alice S. BoothORCID; Charles J. LawORCID; Arthur D. BosmanORCID; Kamber R. SchwarzORCID; Edwin A. BerginORCID; Karin I. ÖbergORCID; Sean M. AndrewsORCID; Viviana V. GuzmánORCID; Catherine WalshORCID; Chunhua QiORCID; Merel L. R. van ’t HoffORCID; Feng LongORCID; David J. WilnerORCID; Jane HuangORCID; Ian CzekalaORCID; John D. IleeORCID; Gianni CataldiORCID; Jennifer B. BergnerORCID; Yuri AikawaORCID; Richard TeagueORCID; Jaehan BaeORCID; Ryan A. LoomisORCID; Jenny K. CalahanORCID; Felipe AlarcónORCID; François MénardORCID; Romane Le GalORCID; Anibal SierraORCID; Yoshihide YamatoORCID; Hideko NomuraORCID; Takashi TsukagoshiORCID; Laura M. PérezORCID; Leon TrapmanORCID; Yao LiuORCID; Kenji FuruyaORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 5

Molecules with ALMA at Planet-forming Scales (MAPS). VI. Distribution of the Small Organics HCN, C2H, and H2CO

Viviana V. GuzmánORCID; Jennifer B. BergnerORCID; Charles J. LawORCID; Karin I. ÖbergORCID; Catherine WalshORCID; Gianni CataldiORCID; Yuri AikawaORCID; Edwin A. BerginORCID; Ian CzekalaORCID; Jane HuangORCID; Sean M. AndrewsORCID; Ryan A. LoomisORCID; Ke ZhangORCID; Romane Le GalORCID; Felipe AlarcónORCID; John D. IleeORCID; Richard TeagueORCID; L. Ilsedore CleevesORCID; David J. WilnerORCID; Feng LongORCID; Kamber R. SchwarzORCID; Arthur D. BosmanORCID; Laura M. PérezORCID; François MénardORCID; Yao LiuORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 6

Molecules with ALMA at Planet-forming Scales (MAPS). VII. Substellar O/H and C/H and Superstellar C/O in Planet-feeding Gas

Arthur D. BosmanORCID; Felipe AlarcónORCID; Edwin A. BerginORCID; Ke ZhangORCID; Merel L. R. van’t HoffORCID; Karin I. ÖbergORCID; Viviana V. GuzmánORCID; Catherine WalshORCID; Yuri AikawaORCID; Sean M. AndrewsORCID; Jennifer B. BergnerORCID; Alice S. BoothORCID; Gianni CataldiORCID; L. Ilsedore CleevesORCID; Ian CzekalaORCID; Kenji FuruyaORCID; Jane HuangORCID; John D. IleeORCID; Charles J. LawORCID; Romane Le GalORCID; Yao LiuORCID; Feng LongORCID; Ryan A. LoomisORCID; François MénardORCID; Hideko NomuraORCID; Chunhua QiORCID; Kamber R. SchwarzORCID; Richard TeagueORCID; Takashi TsukagoshiORCID; Yoshihide YamatoORCID; David J. WilnerORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 7

Molecules with ALMA at Planet-forming Scales (MAPS). VIII. CO Gap in AS 209—Gas Depletion or Chemical Processing?

Felipe AlarcónORCID; Arthur D. BosmanORCID; Edwin A. BerginORCID; Ke ZhangORCID; Richard TeagueORCID; Jaehan BaeORCID; Yuri AikawaORCID; Sean M. AndrewsORCID; Alice S. BoothORCID; Jenny K. CalahanORCID; Gianni CataldiORCID; Ian CzekalaORCID; Jane HuangORCID; John D. IleeORCID; Charles J. LawORCID; Romane Le GalORCID; Yao Liu; Feng LongORCID; Ryan A. LoomisORCID; François MénardORCID; Karin I. ÖbergORCID; Kamber R. SchwarzORCID; Merel L. R. van ’t HoffORCID; Catherine WalshORCID; David J. WilnerORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 8

Molecules with ALMA at Planet-forming Scales (MAPS). IX. Distribution and Properties of the Large Organic Molecules HC3N, CH3CN, and c-C3H2

John D. IleeORCID; Catherine WalshORCID; Alice S. BoothORCID; Yuri AikawaORCID; Sean M. AndrewsORCID; Jaehan BaeORCID; Edwin A. BerginORCID; Jennifer B. BergnerORCID; Arthur D. BosmanORCID; Gianni CataldiORCID; L. Ilsedore CleevesORCID; Ian CzekalaORCID; Viviana V. GuzmánORCID; Jane HuangORCID; Charles J. LawORCID; Romane Le GalORCID; Ryan A. LoomisORCID; François MénardORCID; Hideko NomuraORCID; Karin I. ÖbergORCID; Chunhua QiORCID; Kamber R. SchwarzORCID; Richard TeagueORCID; Takashi TsukagoshiORCID; David J. WilnerORCID; Yoshihide YamatoORCID; Ke ZhangORCID

<jats:title>Abstract</jats:title> <jats:p>The precursors to larger, biologically relevant molecules are detected throughout interstellar space, but determining the presence and properties of these molecules during planet formation requires observations of protoplanetary disks at high angular resolution and sensitivity. Here, we present 0.″3 observations of HC<jats:sub>3</jats:sub>N, CH<jats:sub>3</jats:sub>CN, and <jats:italic>c</jats:italic>-C<jats:sub>3</jats:sub>H<jats:sub>2</jats:sub> in five protoplanetary disks observed as part of the Molecules with ALMA at Planet-forming Scales (MAPS) Large Program. We robustly detect all molecules in four of the disks (GM Aur, AS 209, HD 163296, and MWC 480) with tentative detections of <jats:italic>c</jats:italic>-C<jats:sub>3</jats:sub>H<jats:sub>2</jats:sub> and CH<jats:sub>3</jats:sub>CN in IM Lup. We observe a range of morphologies—central peaks, single or double rings—with no clear correlation in morphology between molecule or disk. Emission is generally compact and on scales comparable with the millimeter dust continuum. We perform both disk-integrated and radially resolved rotational diagram analysis to derive column densities and rotational temperatures. The latter reveals 5–10 times more column density in the inner 50–100 au of the disks when compared with the disk-integrated analysis. We demonstrate that CH<jats:sub>3</jats:sub>CN originates from lower relative heights in the disks when compared with HC<jats:sub>3</jats:sub>N, in some cases directly tracing the disk midplane. Finally, we find good agreement between the ratio of small to large nitriles in the outer disks and comets. Our results indicate that the protoplanetary disks studied here are host to significant reservoirs of large organic molecules, and that this planet- and comet-building material can be chemically similar to that in our own solar system. This paper is part of the MAPS special issue of the Astrophysical Journal Supplement.</jats:p>

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 9

Molecules with ALMA at Planet-forming Scales (MAPS). X. Studying Deuteration at High Angular Resolution toward Protoplanetary Disks

Gianni CataldiORCID; Yoshihide YamatoORCID; Yuri AikawaORCID; Jennifer B. BergnerORCID; Kenji FuruyaORCID; Viviana V. GuzmánORCID; Jane HuangORCID; Ryan A. LoomisORCID; Chunhua QiORCID; Sean M. AndrewsORCID; Edwin A. BerginORCID; Alice S. BoothORCID; Arthur D. BosmanORCID; L. Ilsedore CleevesORCID; Ian CzekalaORCID; John D. IleeORCID; Charles J. LawORCID; Romane Le GalORCID; Yao LiuORCID; Feng LongORCID; François MénardORCID; Hideko NomuraORCID; Karin I. ÖbergORCID; Kamber R. SchwarzORCID; Richard TeagueORCID; Takashi TsukagoshiORCID; Catherine WalshORCID; David J. WilnerORCID; Ke ZhangORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 10

Molecules with ALMA at Planet-forming Scales (MAPS). XI. CN and HCN as Tracers of Photochemistry in Disks

Jennifer B. BergnerORCID; Karin I. ÖbergORCID; Viviana V. GuzmánORCID; Charles J. LawORCID; Ryan A. LoomisORCID; Gianni CataldiORCID; Arthur D. BosmanORCID; Yuri AikawaORCID; Sean M. AndrewsORCID; Edwin A. BerginORCID; Alice S. BoothORCID; L. Ilsedore CleevesORCID; Ian CzekalaORCID; Jane HuangORCID; John D. IleeORCID; Romane Le GalORCID; Feng LongORCID; Hideko NomuraORCID; François MénardORCID; Chunhua QiORCID; Kamber R. SchwarzORCID; Richard TeagueORCID; Takashi TsukagoshiORCID; Catherine WalshORCID; David J. WilnerORCID; Yoshihide YamatoORCID

<jats:title>Abstract</jats:title> <jats:p>UV photochemistry in the surface layers of protoplanetary disks dramatically alters their composition relative to previous stages of star formation. The abundance ratio CN/HCN has long been proposed to trace the UV field in various astrophysical objects; however, to date the relationship between CN, HCN, and the UV field in disks remains ambiguous. As part of the ALMA Large Program MAPS (Molecules with ALMA at Planet-forming Scales), we present observations of CN <jats:italic>N</jats:italic> = 1–0 transitions at 0.″3 resolution toward five disk systems. All disks show bright CN emission within ∼50–150 au, along with a diffuse emission shelf extending up to 600 au. In all sources we find that the CN/HCN column density ratio increases with disk radius from about unity to 100, likely tracing increased UV penetration that enhances selective HCN photodissociation in the outer disk. Additionally, multiple millimeter dust gaps and rings coincide with peaks and troughs, respectively, in the CN/HCN ratio, implying that some millimeter substructures are accompanied by changes to the UV penetration in more elevated disk layers. That the CN/HCN ratio is generally high (&gt;1) points to a robust photochemistry shaping disk chemical compositions and also means that CN is the dominant carrier of the prebiotically interesting nitrile group at most disk radii. We also find that the local column densities of CN and HCN are positively correlated despite emitting from vertically stratified disk regions, indicating that different disk layers are chemically linked. This paper is part of the MAPS special issue of the Astrophysical Journal Supplement.</jats:p>

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 11

Molecules with ALMA at Planet-forming Scales (MAPS). XII. Inferring the C/O and S/H Ratios in Protoplanetary Disks with Sulfur Molecules

Romane Le GalORCID; Karin I. ÖbergORCID; Richard TeagueORCID; Ryan A. LoomisORCID; Charles J. LawORCID; Catherine WalshORCID; Edwin A. BerginORCID; François MénardORCID; David J. WilnerORCID; Sean M. AndrewsORCID; Yuri AikawaORCID; Alice S. BoothORCID; Gianni CataldiORCID; Jennifer B. BergnerORCID; Arthur D. BosmanORCID; L. Ilse CleevesORCID; Ian CzekalaORCID; Kenji FuruyaORCID; Viviana V. GuzmánORCID; Jane HuangORCID; John D. IleeORCID; Hideko NomuraORCID; Chunhua QiORCID; Kamber R. SchwarzORCID; Takashi TsukagoshiORCID; Yoshihide YamatoORCID; Ke ZhangORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 12

Molecules with ALMA at Planet-forming Scales (MAPS). XIII. HCO+ and Disk Ionization Structure

Yuri AikawaORCID; Gianni CataldiORCID; Yoshihide YamatoORCID; Ke ZhangORCID; Alice S. BoothORCID; Kenji FuruyaORCID; Sean M. AndrewsORCID; Jaehan BaeORCID; Edwin A. BerginORCID; Jennifer B. BergnerORCID; Arthur D. BosmanORCID; L. Ilsedore CleevesORCID; Ian CzekalaORCID; Viviana V. GuzmánORCID; Jane HuangORCID; John D. IleeORCID; Charles J. LawORCID; Romane Le GalORCID; Ryan A. LoomisORCID; François MénardORCID; Hideko NomuraORCID; Karin I. ÖbergORCID; Chunhua QiORCID; Kamber R. SchwarzORCID; Richard TeagueORCID; Takashi TsukagoshiORCID; Catherine WalshORCID; David J. WilnerORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 13

Molecules with ALMA at Planet-forming Scales (MAPS). XIV. Revealing Disk Substructures in Multiwavelength Continuum Emission

Anibal SierraORCID; Laura M. PérezORCID; Ke ZhangORCID; Charles J. LawORCID; Viviana V. GuzmánORCID; Chunhua QiORCID; Arthur D. BosmanORCID; Karin I. ÖbergORCID; Sean M. AndrewsORCID; Feng LongORCID; Richard TeagueORCID; Alice S. BoothORCID; Catherine WalshORCID; David J. WilnerORCID; François MénardORCID; Gianni CataldiORCID; Ian CzekalaORCID; Jaehan BaeORCID; Jane HuangORCID; Jennifer B. BergnerORCID; John D. IleeORCID; Myriam BenistyORCID; Romane Le GalORCID; Ryan A. LoomisORCID; Takashi TsukagoshiORCID; Yao LiuORCID; Yoshihide YamatoORCID; Yuri AikawaORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 14