Hillenbrand, Lynne A. and Carpenter, John M. and Skrutskie, M. F. (2001) Periodic Photometric Variability in the Becklin-Neugebauer Object. Astrophysical Journal, 547 (1). L53-L56. ISSN 0004-637X. doi:10.1086/318884. https://resolver.caltech.edu/CaltechAUTHORS:20170516-105658815
![]() |
PDF
- Published Version
See Usage Policy. 57kB |
![]() |
PDF
- Submitted Version
See Usage Policy. 100kB |
Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20170516-105658815
Abstract
The Becklin-Neugebauer object (BN) in the Orion Nebula cluster is a well-studied, optically invisible, infrared-bright young stellar object that is thought to be an intermediate-mass protostar. We report here that BN exhibited nearly sinusoidal periodic variability at the near-infrared H and K_s bands during a 1 month observing campaign in 2000 March/April. The period was 8.28 days, and the peak-to-peak amplitude was ~0.2 mag. Plausible mechanisms for producing the observed variability characteristics are explored.
Item Type: | Article | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Related URLs: |
| ||||||||||||
ORCID: |
| ||||||||||||
Additional Information: | © 2001 The American Astronomical Society. Received 2000 September 1; accepted 2000 November 1; published 2001 January 18. This publication made use of data products from 2MASS, which is funded by NASA and the NSF and is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center at Caltech. Science data and information services were provided by IRSA at IPAC. The authors would like to thank the 2MASS Observatory Staff and Data Management Team for acquiring and pipeline-processing the special survey observations used in this investigation. We thank Nick Scoville, Bill Herbst, Michael Meyer, and Roc Cutri for comments on drafts of this manuscript. We also thank Gerry Neugebauer for communicating previously unpublished data. | ||||||||||||
Group: | Infrared Processing and Analysis Center (IPAC) | ||||||||||||
Funders: |
| ||||||||||||
Subject Keywords: | infrared: stars—stars: individual (Orion BN/KL)—stars: pre–main-sequence—stars: variables: other | ||||||||||||
Issue or Number: | 1 | ||||||||||||
DOI: | 10.1086/318884 | ||||||||||||
Record Number: | CaltechAUTHORS:20170516-105658815 | ||||||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20170516-105658815 | ||||||||||||
Official Citation: | Lynne A. Hillenbrand et al 2001 ApJ 547 L53 | ||||||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||
ID Code: | 77497 | ||||||||||||
Collection: | CaltechAUTHORS | ||||||||||||
Deposited By: | Tony Diaz | ||||||||||||
Deposited On: | 16 May 2017 18:47 | ||||||||||||
Last Modified: | 15 Nov 2021 17:31 |
Repository Staff Only: item control page