The Spitzer C2D Survey of Large, Nearby, Interstellar Clouds. XI. Lupus Observed With IRAC and MIPS
dc.contributor.utaustinauthor | Evans, Neal J., II | en_US |
dc.contributor.utaustinauthor | Harvey, Paul M. | en_US |
dc.creator | Merin, Bruno | en_US |
dc.creator | Jorgensen, Jes | en_US |
dc.creator | Spezzi, Loredana | en_US |
dc.creator | Alcala, Juan M. | en_US |
dc.creator | Evans, Neal J., II | en_US |
dc.creator | Harvey, Paul M. | en_US |
dc.creator | Prusti, Timo | en_US |
dc.creator | Chapman, Nicholas | en_US |
dc.creator | Huard, Tracy | en_US |
dc.creator | van Dishoeck, Ewine F. | en_US |
dc.creator | Comeron, Fernando | en_US |
dc.date.accessioned | 2016-10-28T19:36:22Z | |
dc.date.available | 2016-10-28T19:36:22Z | |
dc.date.issued | 2008-08 | en_US |
dc.description.abstract | We present c2d Spitzer IRAC observations of the Lupus I, III, and IV dark clouds and discuss them in combination with optical, near-infrared, and c2d MIPS data. With the Spitzer data, the new sample contains 159 stars, 4 times larger than the previous one. It is dominated by low- and very low mass stars, and it is complete down to M approximate to 0.1 M-circle dot. We find 30%-40% binaries with separations between 100 and 2000 AU with no apparent effect on the disk properties of the members. A large majority of the objects are Class II or III objects, with only 20 (12%) Class I or flat-spectrum sources. The disk sample is complete down to "debris" -like systems in stars as small as M approximate to 0.2 M-circle dot and includes substellar objects with larger IR excesses. The disk fraction in Lupus is 70%-80%, consistent with an age of 1-2 Myr. However, the young population contains 20% optically thick accretion disks and 40% relatively less flared disks. A growing variety of inner disk structures is found for larger inner disk clearings for equal disk masses. Lupus III is themost centrally populated and rich, followed by Lupus I with a filamentary structure and by Lupus IV, where a very high density core with little star Formation activity has been found. We estimate star Formation rates in Lupus of 2-10 M-circle dot Myr(-1) and star Formation efficiencies of a few percent, apparently correlated with the associated cloud masses. | en_US |
dc.description.department | Astronomy | en_US |
dc.description.sponsorship | NASA 1256316, 1224608, 1230780, 1407 | en_US |
dc.description.sponsorship | Jet Propulsion Laboratory | en_US |
dc.description.sponsorship | California Institute of Technology | en_US |
dc.description.sponsorship | NWO Spinoza | en_US |
dc.description.sponsorship | European Research Training Network HPRN-CT-2002-00308 | en_US |
dc.identifier | doi:10.15781/T2PR7MX02 | |
dc.identifier.citation | Merín, Bruno, Jes Jørgensen, Loredana Spezzi, Juan M. Alcalá, Neal J. Evans II, Paul M. Harvey, Timo Prusti et al. "The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. XI. Lupus Observed With IRAC and MIPS." The Astrophysical Journal Supplement Series, Vol. 177, No. 2 (Aug., 2008): 551. | en_US |
dc.identifier.doi | 10.1086/588042 | en_US |
dc.identifier.issn | 0067-0049 | en_US |
dc.identifier.uri | http://hdl.handle.net/2152/43016 | |
dc.language.iso | English | en_US |
dc.relation.ispartof | en_US | |
dc.relation.ispartofserial | Astrophysical Journal Supplement Series | en_US |
dc.rights | Administrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University. | en_US |
dc.rights.restriction | Open | en_US |
dc.subject | infrared: general | en_US |
dc.subject | ism: individual (lupus i, lupus iii, lupus iv) | en_US |
dc.subject | stars: Formation | en_US |
dc.subject | stars: pre-main-sequence | en_US |
dc.subject | main-sequence stars | en_US |
dc.subject | t-tauri stars | en_US |
dc.subject | low-mass stars | en_US |
dc.subject | spectral | en_US |
dc.subject | energy-distributions | en_US |
dc.subject | young stellar objects | en_US |
dc.subject | southern dark clouds | en_US |
dc.subject | herbig-haro objects | en_US |
dc.subject | array camera irac | en_US |
dc.subject | space-telescope | en_US |
dc.subject | brown dwarfs | en_US |
dc.subject | astronomy & astrophysics | en_US |
dc.title | The Spitzer C2D Survey of Large, Nearby, Interstellar Clouds. XI. Lupus Observed With IRAC and MIPS | en_US |
dc.type | Article | en_US |