Star formation in the Milky Way and nearby galaxies
RC Kennicutt Jr, NJ Evans - Annual Review of Astronomy and …, 2012 - annualreviews.org
We review progress over the past decade in observations of large-scale star formation, with
a focus on the interface between extragalactic and Galactic studies. Methods of measuring …
a focus on the interface between extragalactic and Galactic studies. Methods of measuring …
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 …
X-shooter spectroscopy of young stellar objects-IV. Accretion in low-mass stars and substellar objects in Lupus
JM Alcalá, A Natta, CF Manara, L Spezzi… - Astronomy & …, 2014 - aanda.org
We present VLT/X-shooter observations of a sample of 36 accreting low-mass stellar and
substellar objects (YSOs) in the Lupus star-forming region, spanning a range in mass from …
substellar objects (YSOs) in the Lupus star-forming region, spanning a range in mass from …
The Ophiuchus DIsc Survey Employing ALMA (ODISEA)–I: project description and continuum images at 28 au resolution
LA Cieza, D Ruíz-Rodríguez, A Hales… - Monthly Notices of …, 2019 - academic.oup.com
Abstract We introduce the Ophiuchus DIsc Survey Employing ALMA (ODISEA), a project
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …
HST spectral map** of L/T transition brown dwarfs reveals cloud thickness variations
D Apai, J Radigan, E Buenzli, A Burrows… - The Astrophysical …, 2013 - iopscience.iop.org
Most directly imaged giant exoplanets are fainter than brown dwarfs with similar spectra. To
explain their relative underluminosity, unusually cloudy atmospheres have been proposed …
explain their relative underluminosity, unusually cloudy atmospheres have been proposed …
The Stellar Population of the Chamaeleon I Star-forming Region
KL Luhman - The Astrophysical Journal Supplement Series, 2007 - iopscience.iop.org
ABSTRACT I present a new census of the stellar population in the Chamaeleon I star-
forming region. Using optical and near-IR photometry and follow-up spectroscopy, I have …
forming region. Using optical and near-IR photometry and follow-up spectroscopy, I have …
Characterizing young brown dwarfs using low-resolution near-infrared spectra
Abstract We present near-infrared (1.0-2.4 μm) spectra confirming the youth and cool
temperatures of six brown dwarfs and low-mass stars with circumstellar disks toward the …
temperatures of six brown dwarfs and low-mass stars with circumstellar disks toward the …
The Spitzer Infrared Spectrograph Survey of T Tauri Stars in Taurus
E Furlan, KL Luhman, C Espaillat… - The Astrophysical …, 2011 - iopscience.iop.org
ABSTRACT We present 161 Spitzer Infrared Spectrograph (IRS) spectra of T Tauri stars and
young brown dwarfs in the Taurus star-forming region. All of the targets were selected based …
young brown dwarfs in the Taurus star-forming region. All of the targets were selected based …
The disk population of the Chamaeleon I star-forming region
KL Luhman, LE Allen, PR Allen… - The Astrophysical …, 2008 - iopscience.iop.org
We present a census of circumstellar disks in the Chamaeleon I star-forming region. Using
the Infrared Array Camera and the Multiband Imaging Photometer on board the Spitzer …
the Infrared Array Camera and the Multiband Imaging Photometer on board the Spitzer …
Demographics of disks around young very low-mass stars and brown dwarfs in Lupus
E Sanchis, L Testi, A Natta, CF Manara… - Astronomy & …, 2020 - aanda.org
We present new 890 μm continuum ALMA observations of five brown dwarfs (BDs) with
infrared excess in Lupus I and III, which in combination with four previously observed BDs …
infrared excess in Lupus I and III, which in combination with four previously observed BDs …