Dust evolution and the formation of planetesimals

T Birnstiel, M Fang, A Johansen - Space Science Reviews, 2016 - Springer
The solid content of circumstellar disks is inherited from the interstellar medium: dust
particles of at most a micrometer in size. Protoplanetary disks are the environment where …

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 …

The spitzer space telescope survey of the Orion A and B molecular clouds. I. A census of dusty young stellar objects and a study of their mid-infrared variability

ST Megeath, R Gutermuth, J Muzerolle… - The Astronomical …, 2012 - iopscience.iop.org
We present a survey of the Orion A and B molecular clouds undertaken with the IRAC and
MIPS instruments on board Spitzer. In total, five distinct fields were mapped, covering 9 deg …

Exploration of photothermal sensors based on photothermally responsive materials: a brief review

S Xu, X Bai, L Wang - Inorganic Chemistry Frontiers, 2018 - pubs.rsc.org
The exploration of novel platforms for highly sensitive and selective detection of species of
interest is always demanding. Photothermal sensors have emerged as a novel type of …

A spitzer survey of young stellar clusters within one kiloparsec of the sun: cluster core extraction and basic structural analysis

RA Gutermuth, ST Megeath, PC Myers… - The Astrophysical …, 2009 - iopscience.iop.org
We present a uniform mid-infrared imaging and photometric survey of 36 young, nearby, star-
forming clusters and groups using Spitzer IRAC and MIPS. We have confidently identified …

VOSA: virtual observatory SED analyzer-An application to the Collinder 69 open cluster

A Bayo, C Rodrigo, DB y Navascués, E Solano… - Astronomy & …, 2008 - aanda.org
Context. The physical properties of almost any kind of astronomical object can be derived by
fitting synthetic spectra or photometry extracted from theoretical models to observational …

Interpreting spectral energy distributions from young stellar objects. II. Fitting observed SEDs using a large grid of precomputed models

TP Robitaille, BA Whitney… - The Astrophysical …, 2007 - iopscience.iop.org
We present a method to analyze the spectral energy distributions (SEDs) of young stellar
objects (YSOs). Our approach is to fit data with precomputed two-dimensional (2D) radiation …

Interpreting spectral energy distributions from young stellar objects. I. A grid of 200,000 YSO model SEDs

TP Robitaille, BA Whitney, R Indebetouw… - The Astrophysical …, 2006 - iopscience.iop.org
We present a grid of radiation transfer models of axisymmetric young stellar objects (YSOs),
covering a wide range of stellar masses (from 0.1 to 50 M☉) and evolutionary stages (from …

An observational perspective of transitional disks

C Espaillat, J Muzerolle, J Najita, S Andrews… - arXiv preprint arXiv …, 2014 - arxiv.org
Transitional disks are objects whose inner disk regions have undergone substantial
clearing. The Spitzer Space Telescope produced detailed spectral energy distributions …

Filamentary structure of star-forming complexes

PC Myers - The Astrophysical Journal, 2009 - iopscience.iop.org
The nearest young stellar groups are associated with" hubs" of column density exceeding 10
22 cm− 2, according to recent observations. These hubs radiate multiple" filaments" of …