J 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

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.

Přiložené soubory