J-PLUS: Spectral evolution of white dwarfs by PDF analysis

被引:19
|
作者
Lopez-Sanjuan, C. [1 ]
Tremblay, P-E [2 ]
Ederoclite, A. [3 ]
Ramio, H. Vazquez [1 ]
Carrasco, J. M. [4 ]
Varela, J. [1 ]
Cenarro, A. J. [1 ]
Marin-Franch, A. [1 ]
Civera, T. [1 ]
Daflon, S. [5 ]
Gansicke, B. T. [2 ]
Fusillo, N. P. Gentile [6 ]
Jimenez-Esteban, F. M. [7 ,8 ]
Alcaniz, J. [5 ]
Angulo, R. E. [9 ,10 ]
Cristobal-Hornillos, D. [1 ]
Dupke, R. A. [5 ,11 ,12 ]
Hernandez-Monteagudo, C. [13 ,14 ]
Moles, M. [1 ]
Sodre, L., Jr. [3 ]
机构
[1] Ctr Estudios Fis Cosmos Aragon CEFCA, Unidad Asociada CSIC, Plaza San Juan 1, Teruel 44001, Spain
[2] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
[3] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, BR-05508090 Sao Paulo, Brazil
[4] Univ Barcelona IEEC UB, Inst Ciencies Cosmos, Marti i Franques 1, Barcelona 08028, Spain
[5] Observ Nacl MCTI ON, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, Brazil
[6] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
[7] Ctr Astrobiol CSIC INTA, ESAC Campus,Camino Bajo Castillo S-N, Villanueva De La Canada 28692, Spain
[8] Spanish Virtual Observ, Villanueva De La Canada 28692, Spain
[9] Donostia Int Phys Ctr DIPC, Paseo Manuel de Lardizabal 4, Donostia San Sebastian 20018, Spain
[10] Basque Fdn Sci, Ikerbasque, Bilbao 48013, Spain
[11] Univ Michigan, Dept Astron, 1085 South Univ Ave, Ann Arbor, MI 48109 USA
[12] Univ Alabama, Dept Phys & Astron, Gallalee Hall, Tuscaloosa, AL 35401 USA
[13] Inst Astrofis Canarias, Tenerife 38205, Spain
[14] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
基金
欧盟地平线“2020”; 美国国家科学基金会; 奥地利科学基金会; 美国安德鲁·梅隆基金会; 欧洲研究理事会;
关键词
white dwarfs; methods: statistical; DATA RELEASE; SKY-SURVEY; SPECTROSCOPIC ANALYSIS; LUMINOSITY FUNCTION; HYDROGEN; CATALOG; HELIUM; DA; EXCESS; MASS;
D O I
10.1051/0004-6361/202141746
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. We estimated the spectral evolution of white dwarfs with effective temperature using the Javalambre Photometric Local Universe Survey (J-PLUS) second data release (DR2), which provides 12 photometric optical passbands over 2176 deg(2). Methods. We analyzed 5926 white dwarfs with r <= 19.5 mag in common between a white dwarf catalog defined from Gaia EDR3 and J-PLUS DR2. We performed a Bayesian analysis by comparing the observed J-PLUS photometry with theoretical models of hydrogen- and helium-dominated atmospheres. We estimated the probability distribution functions for effective temperature (T-eff), surface gravity, parallax, and composition; and the probability of having a H-dominated atmosphere (p(H)) for each source. We applied a prior in parallax, using Gaia EDR3 measurements as a reference, and derived a self-consistent prior for the atmospheric composition as a function of T-eff. Results. We described the fraction of white dwarfs with a He-dominated atmosphere (f(He)) with a linear function of the effective temperature at 5000 < T-eff < 30 000 K. We find f(He) = 0.24 +/- 0.01 at T-eff = 10 000 K, a change rate along the cooling sequence of 0.14 +/- 0.02 per 10 kK, and a minimum He-dominated fraction of 0.08 +/- 0.02 at the high-temperature end. We tested the obtained p(H) by comparison with spectroscopic classifications, finding that it is reliable. We estimated the mass distribution for the 351 sources with distance d < 100 pc, mass M > 0.45 M-circle dot, and T-eff > 6000 K. The result for H-dominated white dwarfs agrees with previous studies, with a dominant M = 0.59 M-circle dot peak and the presence of an excess at M similar to 0.8 M-circle dot. This high-mass excess is absent in the He-dominated distribution, which presents a single peak. Conclusions. The J-PLUS optical data provide a reliable statistical classification of white dwarfs into H- and He-dominated atmospheres. We find a 21 +/- 3% increase in the fraction of He-dominated white dwarfs from T-eff = 20 000K to T-eff = 5000 K.
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页数:17
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