CaltechAUTHORS
  A Caltech Library Service

Predicted colors and flux densities of protostars in the Herschel PACS and SPIRE filters

Ali, B. and Tobin, J. J. and Fischer, W. J. and Poteet, C. A. and Megeath, S. T. and Allen, L. and Hartmann, L. and Calvet, N. and Furlan, E. and Osorio, M. (2010) Predicted colors and flux densities of protostars in the Herschel PACS and SPIRE filters. Astronomy and Astrophysics, 518 . Art. No. L119 . ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20101124-081345913

[img]
Preview
PDF - Published Version
See Usage Policy.

551Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20101124-081345913

Abstract

Upcoming surveys with the Herschel Space Observatory will yield far-IR photometry of large samples of young stellar objects, which will require careful interpretation. We investigate the color and luminosity diagnostics based on Herschel broad-band filters to identify and discern the properties of low-mass protostars. We compute a grid of 2016 protostars in various physical congurations, present the expected flux densities and flux density ratios for this grid of protostars, and compare Herschel observations of three protostars to the model results. These provide useful constraints on the range of colors and fluxes of protostar in the Herschel filters. We find that Herschel data alone is likely a useful diagnostic of the envelope properties of young stars.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1051/0004-6361/201014599 DOIArticle
ORCID:
AuthorORCID
Tobin, J. J.0000-0002-6195-0152
Fischer, W. J.0000-0002-3747-2496
Poteet, C. A.0000-0003-4845-7483
Megeath, S. T.0000-0001-7629-3573
Hartmann, L.0000-0003-1430-8519
Calvet, N.0000-0002-3950-5386
Furlan, E.0000-0001-9800-6248
Additional Information:© ESO 2010. Received 31 March 2010; Accepted 27 April 2010. Published online 16 July 2010. Herschel is an ESA space observatory with science instruments provided by Principal Investigator consortia. It is open for proposals for observing time from the worldwide astronomical community. We thank B. Whitney for making her code available publicly. B. Ali acknowledges support from NASA grant IPAC.ALI-OTKP-1- JPL.000094. J. J. Tobin acknowledges support from NASA grant HST-GO- 11548.04-A.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASAHST-GO-11548.04-A
NASAIPAC.ALI-OTKP-1-JPL.000094
Subject Keywords:stars: protostars; radiative transfer; submillimeter: stars
Record Number:CaltechAUTHORS:20101124-081345913
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20101124-081345913
Official Citation:Predicted colors and flux densities of protostars in the Herschel PACS and SPIRE filters B. Ali, J. J. Tobin, W. J. Fischer, C. A. Poteet, S. T. Megeath, L. Allen, L. Hartmann, N. Calvet, E. Furlan and M. Osorio A&A 518 L119 (2010) DOI: 10.1051/0004-6361/201014599
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:21009
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:24 Nov 2010 18:56
Last Modified:07 Nov 2019 00:36

Repository Staff Only: item control page