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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/46HAAD8
Repositorysid.inpe.br/mtc-m21d/2022/03.18.12.37
Last Update2022:03.18.12.37.33 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/03.18.12.37.33
Metadata Last Update2023:01.03.16.46.02 (UTC) administrator
DOI10.1093/mnras/stab3449
ISSN0035-8711
1365-2966
Citation KeyPalaGBPMSBKSSTBBCMGKKLMMNNOPPRRSST:2022:CoEvCa
TitleConstraining the evolution of cataclysmic variables via the masses and accretion rates of their underlying white dwarfs
Year2022
MonthFeb.
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3907 KiB
2. Context
Author 1 Pala, Anna F.
 2 Gänsicke, B. T.
 3 Belloni, Diogo Teixeira
 4 Parsons, S. G.
 5 Marsh, T. R.
 6 Schreiber, M. R.
 7 Breedt, E.
 8 Knigge, C.
 9 Sion, E. M.
10 Szkody, P.
11 Townsley, D.
12 Bildsten, L.
13 Boyd, D.
14 Cook, M. J.
15 De Martino, D.
16 Godon, P.
17 Kafka, S.
18 Kouprianov, V.
19 Long, K. S.
20 Monard, B.
21 Myers, G.
22 Nelson, P.
23 Nogami, D.
24 Oksanen, A.
25 Pickard, R.
26 Poyner, G.
27 Reichart, D. E.
28 Rodriguez Perez, D.
29 Shears, J.
30 Stubbings, R.
31 Toloza, O.
ORCID 1 0000-0001-7069-7403
 2 0000-0002-2761-3005
 3 0000-0003-1535-0866
 4 0000-0002-2695-2654
 5 0000-0002-2498-7589
 6
 7 0000-0001-6180-3438
 8
 9
10
11
12
13
14
15 0000-0002-5069-4202
16 0000-0002-4806-5319
Group 1
 2
 3 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation 1 European Space Agency
 2 University of Warwick
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 University of Sheffield
 5 University of Warwick
 6 Universidad Técnica Federico Santa María
 7 University of Cambridge
 8 University of Southampton
 9 Villanova University
10 University of Washington
11 University of Alabama
12 University of California, Santa Barbara
13 British Astronomical Association
14 American Association of Variable Star Observers
15 Osservatorio Astronomico di Capodimonte
16 Villanova University
17 American Association of Variable Star Observers
18 University of North Carolina at Chapel Hill
19 Space Telescope Science Institut
20 CBA Kleinkaroo
21 American Association of Variable Star Observers
22 American Association of Variable Star Observers
23 Kyoto University
24 Hankasalmi Observatory
25 British Astronomical Association
26 British Astronomical Association
27 University of North Carolina at Chapel Hill
28 American Association of Variable Star Observers
29 British Astronomical Association
30 American Association of Variable Star Observers
31 Universidad Técnica Federico Santa María
Author e-Mail Address 1 annafpala@gmail.com
 2
 3 diogobellonizorzi@gmail.com
JournalMonthly Notices of the Royal Astronomical Society
Volume510
Number4
Pages6110-6132
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV
History (UTC)2022-03-18 12:37:33 :: simone -> administrator ::
2022-03-18 12:37:34 :: administrator -> simone :: 2022
2022-03-18 12:45:18 :: simone -> administrator :: 2022
2023-01-03 16:46:02 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsstars: white dwarfs
cataclysmic variables
evolution
fundamental parameters
AbstractWe report on the masses (M-WD), effective temperatures (T-eff), and secular mean accretion rates (< M >) of 43 cataclysmic variable (CV) white dwarfs, 42 of which were obtained from the combined analysis of their Hubble Space Telescope ultraviolet data with the parallaxes provided by the Early Third Data Release of the Gaia space mission, and one from the white dwarf gravitational redshift. Our results double the number of CV white dwarfs with an accurate mass measurement, bringing the total census to 89 systems. From the study of the mass distribution, we derive < M-WD > = 0.81(-0.20)(+0.16) M-circle dot, in perfect agreement with previous results, and find no evidence of any evolution of the mass with orbital period. Moreover, we identify five systems with M-WD < 0.5 M-circle dot, which are most likely representative of helium-core white dwarfs, showing that these CVs are present in the overall population. We reveal the presence of an anticorrelation between the average accretion rates and the white dwarf masses for the systems below the 2-3 h period gap. Since <(M) over dot > reflects the rate of system angular momentum loss, this correlation suggests the presence of an additional mechanism of angular momentum loss that is more efficient at low white dwarf masses. This is the fundamental concept of the recently proposed empirical prescription of consequential angular momentum loss (eCAML) and our results provide observational support for it, although we also highlight how its current recipe needs to be refined to better reproduce the observed scatter in T-eff and <(M) over dot >, and the presence of helium-core white dwarfs.
AreaCEA
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zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/46HAAD8
Languageen
Target FilePala_2022_constraining.pdf
User Groupsimone
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simone
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Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
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Next Higher Units8JMKD3MGPCW/46KTFK8
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2021/06.04.03.40
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