Zobrazeno 1 - 10
of 37
pro vyhledávání: '"A. M. Rilinger"'
Autor:
Anneliese M. Rilinger, Catherine C. Espaillat, Zihua Xin, Álvaro Ribas, Enrique Macías, Sarah Luettgen
Publikováno v:
The Astrophysical Journal, Vol 954, Iss 2, p 222 (2023)
Externí odkaz:
https://doaj.org/article/b21fd09548a14cb1aa97899e172d4366
Publikováno v:
The Astrophysical Journal, Vol 947, Iss 2, p 91 (2023)
Externí odkaz:
https://doaj.org/article/009c4a86fb9f4379b4f18ea517950b50
Autor:
Anneliese M. Rilinger, Catherine C. Espaillat, Zihua Xin, Álvaro Ribas, Enrique Macías, Sarah Luettgen
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 1, p 66 (2023)
We present spectral energy distribution (SED) modeling of 338 disks around T Tauri stars from 11 star-forming regions, ranging from ∼0.5 to 10 Myr old. The disk masses we infer from our SED models are typically greater than those reported from (sub
Externí odkaz:
https://doaj.org/article/ba4f3d8450f9418181fcb1effd028d5d
Publikováno v:
The Astrophysical Journal, Vol 942, Iss 1, p 4 (2022)
Accurate disk mass measurements are necessary to constrain disk evolution and the timescale of planet formation, but such measurements are difficult to make and are very dependent on assumptions. Here, we look at the assumption that the disk is optic
Externí odkaz:
https://doaj.org/article/d813f94a2b9042ba834b9fda8d21c4c6
Accurate disk mass measurements are necessary to constrain disk evolution and the timescale of planet formation, but such measurements are difficult to make and are very dependent on assumptions. Here we look at the assumption that the disk is optica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c3c6e225ab6bc0a220ad96cd4ae78b8
https://www.repository.cam.ac.uk/handle/1810/344880
https://www.repository.cam.ac.uk/handle/1810/344880
We present the largest sample of brown dwarf (BD) protoplanetary disk spectral energy distributions modeled to date. We compile 49 objects with ALMA observations from four star-forming regions: $\rho$ Ophiuchus, Taurus, Lupus, and Upper Scorpius. Stu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a621fd90a38571987bf148f3f641d300
Publikováno v:
The Astrophysical Journal. 926:67
Wide-field near-infrared (NIR) polarimetry was used to examine disk systems around two brown dwarfs (BD) and two young stellar objects (YSO) embedded in the Heiles Cloud 2 (HCl2) dark molecular cloud in Taurus as well as numerous stars located behind
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fda9f8939bfdaad19f8cecab9d5c017f
https://doi.org/10.3847/1538-4357/ac415c
https://doi.org/10.3847/1538-4357/ac415c
Measuring the properties of protoplanetary disks around brown dwarfs is central to understanding the formation of brown dwarfs and their planetary companions. We present modeling of CFHT Tau 4 and 2M0444, two brown dwarfs with protoplanetary disks in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7be889243a607abdbc33eb5d9fedb659
http://arxiv.org/abs/1905.05829
http://arxiv.org/abs/1905.05829
Magnetic Inflation and Stellar Mass III: Revised Parameters for the Component Stars of NSVS 07394765
Autor:
Brian F. Healy, Anneliese M. Rilinger, Jonathan J. Swift, Tom Polakis, Eunkyu Han, Philip S. Muirhead, Brian Skiff
We perform a new analysis of the M dwarf-M dwarf eclipsing binary system NSVS 07394765 in order to investigate the reported hyper-inflated radius of one of the component stars. Our analysis is based on archival photometry from the Wide Angle Search f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13b5c6eb3901b197d2e657e9509db805
Autor:
Kyoung Hee Kim, Enrique Macías, William J. Fischer, Sierra L. Grant, John J. Tobin, Álvaro Ribas, Nuria Calvet, John Wendeborn, Catherine Espaillat, Anneliese M. Rilinger, S. Thomas Megeath
Publikováno v:
The Astrophysical Journal. 913:123
We present ALMA observations of 101 protoplanetary disks within the star-forming region Lynds 1641 in the Orion Molecular Cloud A. Our observations include 1.33 mm continuum emission and spectral windows covering the J=2-1 transition of $^{12}$CO, $^
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d8a95c5191119d098aa44fb216b8c323
https://doi.org/10.3847/1538-4357/abf432
https://doi.org/10.3847/1538-4357/abf432