Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
Evolution of debris disks
MC Wyatt - Annu. Rev. Astron. Astrophys., 2008 - annualreviews.org
Circumstellar dust exists around several hundred main sequence stars. For the youngest
stars, that dust could be a remnant of the protoplanetary disk. Mostly it is inferred to be …
stars, that dust could be a remnant of the protoplanetary disk. Mostly it is inferred to be …
A reappraisal of the habitability of planets around M dwarf stars
Stable, hydrogen-burning, M dwarf stars make up about 75% of all stars in the Galaxy. They
are extremely long-lived, and because they are much smaller in mass than the Sun …
are extremely long-lived, and because they are much smaller in mass than the Sun …
The Spitzer c2d legacy results: star-formation rates and efficiencies; evolution and lifetimes
NJ Evans, MM Dunham, JK Jørgensen… - The Astrophysical …, 2009 - iopscience.iop.org
ABSTRACT The c2d Spitzer Legacy project obtained images and photometry with both
IRAC and MIPS instruments for five large, nearby molecular clouds. Three of the clouds …
IRAC and MIPS instruments for five large, nearby molecular clouds. Three of the clouds …
Imaging extrasolar giant planets
BP Bowler - Publications of the Astronomical Society of the …, 2016 - iopscience.iop.org
High-contrast adaptive optics (AO) imaging is a powerful technique to probe the
architectures of planetary systems from the outside-in and survey the atmospheres of self …
architectures of planetary systems from the outside-in and survey the atmospheres of self …
[BOOK][B] Dust in the galactic environment
DCB Whittet - 2018 - taylorfrancis.com
Dust is a ubiquitous feature of the cosmos, im**ing directly or indirectly on most fields of
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …
Planet formation around stars of various masses: the snow line and the frequency of giant planets
We use a semianalytic circumstellar disk model that considers movement of the snow line
through evolution of accretion and the central star to investigate how gas giant frequency …
through evolution of accretion and the central star to investigate how gas giant frequency …
A Spitzer Space Telescope study of disks in the young σ Orionis cluster
J Hernández, L Hartmann, T Megeath… - The Astrophysical …, 2007 - iopscience.iop.org
Abstract We report new Spitzer Space Telescope observations, using the IRAC and MIPS
instruments, of the young (~ 3 Myr) σ Orionis cluster. We identify 336 stars as members of the …
instruments, of the young (~ 3 Myr) σ Orionis cluster. We identify 336 stars as members of the …
The disk population of the Taurus star-forming region
KL Luhman, PR Allen, C Espaillat… - The Astrophysical …, 2009 - iopscience.iop.org
We have analyzed nearly all images of the Taurus star-forming region at 3.6, 4.5, 5.8, 8.0,
and 24 μm that were obtained during the cryogenic mission of the Spitzer Space Telescope …
and 24 μm that were obtained during the cryogenic mission of the Spitzer Space Telescope …
A Census of the Taurus star-forming region and neighboring associations with Gaia
KL Luhman - The Astronomical Journal, 2023 - iopscience.iop.org
I have used high-precision photometry and astrometry from the third data release of Gaia to
perform a survey for members of the Taurus star-forming region and young associations in …
perform a survey for members of the Taurus star-forming region and young associations in …
Debris disk evolution around A stars
We report 24 and/or 70 μm measurements of~ 160 A-type main-sequence stars using the
Multiband Imaging Photometer for Spitzer (MIPS). Their ages range from 5 to 850 Myr …
Multiband Imaging Photometer for Spitzer (MIPS). Their ages range from 5 to 850 Myr …