[HTML][HTML] Pre-main-sequence evolution in the Taurus-Auriga molecular cloud

SJ Kenyon, L Hartmann - … Journal Supplement v. 101, p. 117, 1995 - adsabs.harvard.edu
This paper analyzes optical and infrared photometry of pre-main-sequence stars in the
Taurus-Aunga molecular cloud. More than half of the stars in our sample have excess near …

Intrinsic near-infrared excesses of T Tauri stars: understanding the classical T Tauri star locus

MR Meyer, N Calvet… - … Journal v. 114, p. 288-300 …, 1997 - adsabs.harvard.edu
We re-examine the observed near-infrared properties of T Tauri stars and interpret them with
the aid of accretion disk models. Based upon a careful analysis of the dereddened near …

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 …

Passive irradiated circumstellar disks with an inner hole

CP Dullemond, C Dominik, A Natta - The Astrophysical Journal, 2001 - iopscience.iop.org
ABSTRACT A model for irradiated dust disks around Herbig Ae stars is proposed. The
model is based on the flaring disk model given by Chiang and Goldreich in 1997, but with …

[HTML][HTML] The pre-main-sequence evolution of intermediate-mass stars

F Palla, SW Stahler - Astrophysical Journal v. 418, p. 414, 1993 - adsabs.harvard.edu
The Pre-Main-Sequence Evolution of Intermediate-Mass Stars ADS Classic is now deprecated.
It will be completely retired in October 2019. This page will automatically redirect to the new …

Two-dimensional radiative transfer in protostellar envelopes. I. Effects of geometry on class I sources

BA Whitney, K Wood, JE Bjorkman… - The Astrophysical …, 2003 - iopscience.iop.org
We present two-dimensional radiation transfer models of class I protostars and show the
effect of including more realistic geometries on the resulting spectral energy distributions …

Pre-main-sequence isochrones–II. Revising star and planet formation time-scales

CPM Bell, T Naylor, NJ Mayne… - Monthly Notices of …, 2013 - academic.oup.com
We have derived ages for 13 young (< 30 Myr) star-forming regions and find that they are up
to a factor of 2 older than the ages typically adopted in the literature. This result has wide …

Near-infrared photometric variability of stars toward the Orion A molecular cloud

JM Carpenter, LA Hillenbrand… - The Astronomical …, 2001 - iopscience.iop.org
We present an analysis of J, H, and K s time-series photometry obtained with the southern
2MASS telescope over a 0 &fdg; 84× 6 region centered near the Trapezium region of the …

An ultraviolet, optical and infrared study of Herbig Ae/Be stars

K Malfait, E Bogaert, C Waelkens - … , v. 331, p. 211-223 (1998), 1998 - adsabs.harvard.edu
We have selected a list of 45 Herbig Ae/Be-type candidates on the base of their IRAS colors
and their spectral types. We propose the presence of a broad infrared excess as a defining …