2026
Unraveling the brown dwarf desert: Four new discoveries and a unifying period-coded picture
SUBJAK, Jan; Rafael BRAHM; Jozef LIPTAK; Jan EBERHARDT; Marcelo TALA PINTO et al.Základní údaje
Originální název
Unraveling the brown dwarf desert: Four new discoveries and a unifying period-coded picture
Autoři
SUBJAK, Jan; Rafael BRAHM; Jozef LIPTAK; Jan EBERHARDT; Marcelo TALA PINTO; Sarah L. CASEWELL; Thomas HENNING; Katharine HESSE; Trifon TRIFONOV; Andres JORDAN; Felipe I. ROJAS; Michaela VÍTKOVÁ ORCID; Helem SALINAS; Gavin BOYLE; Vincent SUC; Luca ANTONUCCI; Krzysztof BERNACKI; Cesar BRICENO; Karen A. COLLINS; Jorge FERNANDEZ FERNANDEZ; Samuel GILL; Jan JANÍK ORCID; Nicholas LAW; Andrew W. MANN; James MCCORMAC; Adam POPOWICZ; Daniel SEBASTIAN; Marek SKARKA; Jan VACLAVIK; Leonardo VANZI; Richard G. WEST; Francis P. WILKIN a Carl ZIEGLER
Vydání
ASTRONOMY & ASTROPHYSICS, LES ULIS CEDEX A, EDP SCIENCES S A, 2026, 0004-6361
Další údaje
Jazyk
angličtina
Typ výsledku
Článek v odborném periodiku
Obor
10308 Astronomy
Stát vydavatele
Francie
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Impakt faktor
Impact factor: 5.800 v roce 2024
Označené pro přenos do RIV
Ano
Organizační jednotka
Přírodovědecká fakulta
UT WoS
EID Scopus
Klíčová slova anglicky
techniques: photometric; techniques: radial velocities; techniques: spectroscopic; planets and satellites: formation; planet-disk interactions; brown dwarfs
Štítky
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 16. 7. 2026 12:31, Mgr. Marie Novosadová Šípková, DiS.
Anotace
V originále
We present four newly validated transiting brown dwarfs identified through TESS photometry and confirmed with high-precision radial velocity measurements obtained from the FEROS and PLATOSpec spectrographs. Notably, three of these companions exhibit orbital periods exceeding 100 days, thereby expanding the sample of long-period transiting brown dwarfs from four to seven systems. The host stars of the long-period brown dwarfs show mild subsolar metallicity. These discoveries highlight the expansion of the metal-poor long-period distribution and help us better understand the brown dwarf desert. In our comparative analysis of eccentricity and metallicity demographics, we utilized catalogs of long-period giant planets, brown dwarfs, and low-mass stellar companions. After accounting for tidal influences, the eccentricity distribution aligns with that of low-mass stellar binaries, presenting a different profile than that observed within the giant planet population. Additionally, the metallicity of the host stars reveals a noteworthy trend: Short-period transiting brown dwarfs are predominantly associated with metal-rich stars, whereas long-period brown dwarfs are more often found around metal-poor stars, thus demonstrating statistical similarities to low-mass stellar hosts. This trend has been previously observed in studies of hot and cold Jupiters and points to a period-coded mixture of channels. A natural explanation is that most brown dwarfs originate from fragmentation at wider separations, with long-period systems retaining this stellar-like imprint, while only those embedded in massive, long-lived metal-rich protoplanetary disks are efficiently delivered and stabilized to short orbits.