Far-Infrared Observations of the Very Low Luminosity Embedded Source L1521F-IRS in the Taurus Star-Forming Region

May 2009 • 2009ApJ...696.1918T

Authors • Terebey, Susan • Fich, Michel • Noriega-Crespo, Alberto • Padgett, Deborah L. • Fukagawa, Misato • Audard, Marc • Brooke, Tim • Carey, Sean • Evans, Neal J., II • Guedel, Manuel • Hines, Dean • Huard, Tracy • Knapp, Gillian R. • McCabe, Caer-Eve • Menard, Francois • Monin, Jean-Louis • Rebull, Luisa

Abstract • We investigate the environment of the very low luminosity object L1521F-IRS using data from the Taurus Spitzer Legacy Survey. The MIPS 160 μm image shows both extended emission from the Taurus cloud and emission from multiple cold cores over a 1° × 2° region. Analysis shows that the cloud dust temperature is 14.2 ± 0.4 K and the extinction ratio is A 160/AK = 0.010 ± 0.001 up to AV ~ 4 mag. We find κ160 = 0.23 ± 0.046 cm2 g-1 for the specific opacity of the gas-dust mixture. Therefore, for dust in the Taurus cloud we find that the 160 μm opacity is significantly higher than that measured for the diffuse interstellar medium, but not too different from dense cores, even at modest extinction values. Furthermore, the 160 μm image shows features that do not appear in the IRAS 100 μm image. We identify six regions as cold cores, i.e., colder than 14.2 K, all of which have counterparts in extinction maps or C18O maps. Three of the six cores contain embedded young stellar objects, which demonstrates the cores are sites of current star formation. We compare the effects of L1521F-IRS on its natal core and find there is no evidence for dust heating at 160 or 100 μm by the embedded source. From the infrared luminosity L TIR = 0.024 L sun we find L_bol\_int = 0.034-0.046\;L_{\odot }, thus confirming the source's low luminosity. Comparison of L1521F-IRS with theoretical simulations for the very early phases of star formation appears to rule out the first core collapse phase. The evolutionary state appears similar to or younger than the class 0 phase, and the estimated mass is likely to be substellar.


IPAC Authors

Sean Carey

Senior Scientist


Luisa Rebull

Senior Research Scientist