| Full text | |
| Author(s): Show less - |
David-Uraz, A.
[1]
;
Neiner, C.
[2]
;
Sikora, J.
[3, 4]
;
Bowman, D. M.
[5]
;
Petit, V.
[1]
;
Chowdhury, S.
[6]
;
Handler, G.
[6]
;
Pergeorelis, M.
[1]
;
Cantiello, M.
[7, 8]
;
Cohen, D. H.
[9]
;
Erba, C.
[1]
;
Keszthelyi, Z.
[3, 4]
;
Khalack, V.
[10]
;
Kobzar, O.
[10]
;
Kochukhov, O.
[11]
;
Labadie-Bartz, J.
[12]
;
Lovekin, C. C.
[13]
;
MacInnis, R.
[1]
;
Owocki, S. P.
[1]
;
Pablo, H.
[14]
;
Shultz, M. E.
[1]
;
Ud-Doula, A.
[15]
;
Wade, G. A.
[4]
;
Collaboration, MOBSTER
Total Authors: 24
|
| Affiliation: Show less - | [1] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 - USA
[2] Univ Paris Diderot, Sorbonne Univ, PSL Univ, LESIA, Observ Paris, CNRS, Sorbonne Paris Cite, 5 Pl Jules Janssen, F-92195 Meudon - France
[3] Queens Univ, Dept Phys Engn Phys & Astron, Kingston, ON K7L 3N6 - Canada
[4] Royal Mil Coll Canada, Dept Phys & Space Phys, POB 17000, Kingston, ON K7K 7B4 - Canada
[5] Katholieke Univ Leuven, Inst Sterrenkunde, Celestijnenlaan 200D, B-3001 Leuven - Belgium
[6] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw - Poland
[7] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 - USA
[8] Flatiron Inst, Ctr Computat Astrophys, 162 5th Ave, New York, NY 10010 - USA
[9] Swarthmore Coll, Dept Phys & Astron, Swarthmore, PA 19081 - USA
[10] Univ Moncton, Dept Phys & Astron, Moncton, NB E1A 3E9 - Canada
[11] Uppsala Univ, Dept Phys & Astron, Box 516, SE-75120 Uppsala - Sweden
[12] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, Rua Matao 1226, Cidade Univ, BR-05508900 Sao Paulo, SP - Brazil
[13] Mt Allison Univ, Dept Phys, Sackville, NB E4L 1E6 - Canada
[14] AAVSO Headquarters, 49 Bay State Rd, Cambridge, MA 02138 - USA
[15] Penn State Scranton, 120 Ridge View Dr, Dunmore, PA 18512 - USA
Total Affiliations: 15
|
| Document type: | Journal article |
| Source: | Monthly Notices of the Royal Astronomical Society; v. 487, n. 1, p. 304-317, JUL 2019. |
| Web of Science Citations: | 5 |
| Abstract | |
In this paper we introduce the MOBSTER collaboration and lay out its scientific goals. We present first results based on the analysis of 19 previously known magnetic O, B, and A stars observed in 2-min cadence in sectors 1 and 2 of the Transiting Exoplanet Survey Satellite (TESS) mission. We derive precise rotational periods from the newly obtained light curves and compare them to previously published values. We also discuss the overall photometric phenomenology of the known magnetic massive and intermediate-mass stars and propose an observational strategy to augment this population by taking advantage of the high-quality observations produced by TESS. (AU) | |
| FAPESP's process: | 17/23731-1 - Analysis and Modeling of a Large Sample of Galactic Be Stars |
| Grantee: | Jonathan Michael Labadie-Bartz |
| Support Opportunities: | Scholarships in Brazil - Post-Doctoral |