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Research Notes of the AAS (RNAAS)

Resumen/Descripción – provisto por la editorial en inglés
Research Notes of the AAS is a non-peer reviewed, indexed and secure record of works in progress, comments and clarifications, null results, or timely reports of observations in astronomy and astrophysics.
Palabras clave – provistas por la editorial

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Institución detectada Período Navegá Descargá Solicitá
No detectada desde ene. 2017 / hasta dic. 2023 IOPScience

Información

Tipo de recurso:

revistas

ISSN electrónico

2515-5172

Editor responsable

American Astronomical Society (AAS)

País de edición

Estados Unidos

Información sobre licencias CC

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

Cobertura temática

Tabla de contenidos

Photometry of 10 Million Stars from the First Two Years of TESS Full Frame Images: Part II

Chelsea X. HuangORCID; Andrew VanderburgORCID; Andras PálORCID; Lizhou ShaORCID; Liang YuORCID; Willie Fong; Michael FausnaughORCID; Avi ShporerORCID; Natalia GuerreroORCID; Roland VanderspekORCID; George RickerORCID

Palabras clave: General Medicine.

Pp. 206

Erratum: “A Search for the Guest Star Associated with Swift J1818-5937” (2020, RNAAS, 4, 164)

Yu LiuORCID; Yuan-Chuan ZouORCID

Palabras clave: General Medicine.

Pp. 208

Influence of Neptune’s Migration Parameters on the Inclination Distribution of Kuiper Belt Objects (KBOs)

David NesvornýORCID

<jats:title>Abstract</jats:title> <jats:p>Nesvorný suggested that Neptune’s early migration must have been slow (one <jats:italic>e</jats:italic>-fold <jats:italic>τ</jats:italic> ≳ 10 Myr) to explain the wide inclination distribution of dynamically hot populations in the Kuiper Belt. Volk &amp; Malhotra reported that the median inclination of implanted KBOs, <jats:italic>i</jats:italic> <jats:sub>M</jats:sub>, depends on Neptune’s orbital inclination during migration. They did not find any simple relationship between <jats:italic>i</jats:italic> <jats:sub>M</jats:sub> and <jats:italic>τ</jats:italic> for 5 ≤ <jats:italic>τ</jats:italic> ≤ 50 Myr (very short migration timescales <jats:italic>τ</jats:italic> &lt; 5 Myr can be ruled out; e.g., Figure 2 in Nesvorný). Here we briefly explain—a full account of our research will be published elsewhere—how these seemingly contradictory findings can be reconciled.</jats:p>

Palabras clave: General Medicine.

Pp. 212

WR6: A Rejuvenated Runaway Star

V. V. GvaramadzeORCID

Palabras clave: General Medicine.

Pp. 213

A New Grid of Model Atmospheres for Metal-poor Ultracool Brown Dwarfs

Roman GerasimovORCID; Derek HomeierORCID; Adam BurgasserORCID; Luigi R. Bedin

Palabras clave: General Medicine.

Pp. 214

Blind Prediction of the Returning Image of Supernova Refsdal from a New Lens Model of the Galaxy Cluster MACS J1149.5+2223

Wenlei ChenORCID; Patrick L. Kelly; Liliya L. R. WilliamsORCID

Palabras clave: General Medicine.

Pp. 215

Locating the Alfvénic Speed Transition in the Solar Corona

David B. WexlerORCID; Gavin M. Lawhite; Paul SongORCID

Palabras clave: General Medicine.

Pp. 216

A Word of Caution About Exoplanet Archival Data

Dimitris M. ChristodoulouORCID; Demosthenes KazanasORCID

Palabras clave: General Medicine.

Pp. 217

Impossible Survivors: New Star Cluster Candidates in the Galactic Bulge

Dante MinnitiORCID; Matías Gómez; Joyce B. Pullen; Tali Palma; Juan José Clariá; Javier Alonso-GarcíaORCID; Roberto K. SaitoORCID; Leigh Smith; José G. Fernández-Trincado; Maren Hempel

Palabras clave: General Medicine.

Pp. 218

The Open Cataclysmic Variable Catalog

Ryan JackimORCID; Paula SzkodyORCID; Bryna HazeltonORCID; Noah C. BensonORCID

Palabras clave: General Medicine.

Pp. 219